The galaxy presents as a relatively small, disk-shaped system, exhibiting a moderate degree of inclination with respect to our line of sight. A central bulge is apparent, exhibiting a concentrated luminosity. The disk appears fairly smooth, with no immediately discernible spiral arm structure. There's no evidence of significant recent merger activity or strong tidal features. The overall color index suggests a population of older stars. The lack of prominent blue regions indicates limited ongoing star formation. The galaxy appears to be relatively isolated, showing no clear interaction with any neighboring galaxies in the immediate vicinity.
