The galaxy presents as an elongated, likely disc-shaped structure seen at a high inclination. It displays a generally smooth profile, suggestive of an older stellar population with limited ongoing star formation, though there may be some areas of star formation present. Color gradients are subtle, with a slightly bluer hue in some areas, possibly indicating the presence of younger stars or less dust extinction in those locations. There is little evidence of a strong central bulge or active galactic nucleus in the available image data. There appear to be no obvious signs of major mergers or tidal interactions with other galaxies, but it is possible a minor disturbance is present. Overall, the galaxy appears to be a relatively undisturbed, mid-sized system.
