The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a notable central bulge with a smooth, diffused light distribution.  The bulge dominates the overall luminosity profile, suggesting an older stellar population.  A faint, flattened disk component may be present, though its features are not well-defined, showing minimal spiral arm structure. The galaxy's color index is redder in the bulge and slightly bluer in the faint disk, hinting at ongoing, albeit low, star formation in the outer regions. The shape is generally ellipsoidal.  There is no clear evidence of strong tidal interactions or significant morphological disturbances. The galaxy presents a relatively isolated structure.
