The galaxy presents a generally smooth, elliptical morphology. A centrally concentrated bulge dominates the light profile, exhibiting a bright, yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy appear less luminous with a diffuse, less structured halo. A slight elongation is observable, deviating from a perfectly circular shape. There is little evidence of spiral arm structure or dust lanes. A subtle blue tint is noticeable in the fainter, extended regions of the halo, possibly indicating the presence of some younger, hotter stars. The overall appearance is consistent with an early-type galaxy, potentially an elliptical. There is no obvious indication of significant tidal disturbances or ongoing major merger activity, although subtle asymmetries in the outer regions may suggest past interactions. 
