The galaxy presents as a somewhat elliptical, disk-like structure. Its overall light distribution appears relatively smooth. A central bulge region is evident, exhibiting a more concentrated and brighter luminosity. The color profile suggests an older stellar population dominates, with a yellow-red hue concentrated in the core. The outer disk regions show bluer tones implying the presence of some younger, hotter stars and thus some possible star formation. There may be faint indications of spiral arm structure. Overall, the galaxy appears to be fairly isolated, lacking any obvious signs of major ongoing mergers or significant tidal disturbances. There is slight irregularity in the overall shape.
