The galaxy presents an overall smooth morphology, appearing predominantly elliptical in shape with a slight elongation. A central bulge is visible, exhibiting a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a bluer tint compared to the core, hinting at the presence of younger, hotter stars and potentially some ongoing star formation. There are faint indications of minor disturbances in the morphology, potentially due to minor gravitational interactions. No spiral arms or a well-defined disk are apparent, supporting the classification as an elliptical or lenticular galaxy.
