The galaxy presents an overall smooth and rounded morphology. There is evidence of a central bulge, characterized by a high concentration of light. The galaxy's color appears relatively uniform, trending towards redder hues, suggestive of an older stellar population and limited recent star formation. While a disk-like structure is not immediately obvious, the isophotes surrounding the bulge seem slightly elongated, possibly indicating an underlying disk component seen at a relatively high inclination. There are subtle hints of minor disturbances in its overall structure, potentially indicative of a past or ongoing interaction. No clear spiral arm structure is apparent, supporting the observed redder color and a morphology that is more characteristic of early-type galaxies.
