The galaxy presents a generally smooth and rounded morphology, suggestive of an elliptical galaxy.  It displays a concentrated central bulge, with light diffusing outwards into a more indistinct halo. Color gradients are subtle, with the central region exhibiting a slightly yellower hue, indicative of an older stellar population.  There's no obvious spiral arm structure or dust lane visible. Given the overall morphology, star formation activity appears to be low. There is no evidence of any major tidal disturbances or ongoing mergers.
