The galaxy presents as an elongated, lenticular-like structure. The central region displays a bright, concentrated luminosity suggesting a significant stellar population or active galactic nucleus, potentially obscured. The disk exhibits a relatively smooth texture with a noticeable blue hue in the outer regions, possibly indicating ongoing star formation. The bulge seems to dominate the overall light profile, displaying a more yellow/white color, typical of older stellar populations. The disk appears significantly thinner relative to the bulge, with an estimated axis ratio of approximately 0.5. The galaxy appears relatively undisturbed, lacking any obvious signs of recent major mergers or tidal interactions, although there may be minor distortions in the outer disk region. A sersic profile modeling may indicate intermediate concentration and flatten. The color index values show a moderate excess of blue over red when comparing the images from DESI and Legacy surveys. Overall, the galaxy appears to be an intermediate-mass system, undergoing a relatively quiescent phase of evolution.
