The galaxy presents a slightly elongated, lenticular appearance. The central bulge exhibits a smooth, concentrated distribution of light, appearing yellowish-orange in color. This suggests a population of older stars. A faint, extended disk surrounds the bulge, displaying a greenish hue. This color might indicate the presence of ongoing, albeit subdued, star formation activity. The galaxy's overall morphology does not suggest significant recent or ongoing mergers, though a subtle irregularity in the disk's structure may be present. A small amount of tidal disturbances cannot be ruled out. A moderate degree of inclination relative to our line of sight is suspected. 
