The galaxy appears as an elliptical or lenticular-like structure, exhibiting a generally smooth, concentrated light distribution. A pronounced central bulge is apparent, suggesting a concentration of older stars. There is a subtle color gradient, transitioning from a slightly bluer hue at the outer edges to a yellower or redder tone towards the galactic center. The galaxy lacks any discernible spiral arm structure or prominent dust lanes. There are no signs of active galactic nuclei or bright star-forming regions. The overall morphology indicates a relatively evolved galaxy, with a dominant spheroid component and minimal ongoing star formation. The apparent axial ratio suggests a moderate degree of ellipticity. The galaxy seems to be relatively isolated, showing no visual signs of tidal interaction or recent merger events. 
