The galaxy presents as a primarily smooth object with a generally round morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity outwards. There is little evidence of strong spiral arm structure or distinct features like bars. The color gradient suggests an older stellar population, with redder hues dominating the galaxy's light output. There may be some minor indications of tidal disturbances or asymmetry, but the overall appearance suggests a relaxed system.
