The galaxy presents as a relatively smooth, centrally concentrated object. There is a subtle color gradient, with a slightly redder hue towards the center and a bluer tint in the outer regions. Its morphology appears mostly elliptical, though not perfectly so; there is a slight irregularity suggestive of a possible faint disk or tidal feature, although this is uncertain given the image quality. The central bulge region dominates the light profile. There is no clear evidence of strong spiral arm structure or dust lanes. Based on its overall morphology and color profile, it likely represents a relatively massive system with an appreciable stellar population, exhibiting moderate levels of recent or ongoing star formation. There might be weak tidal features, which could indicate past or ongoing interaction with another galaxy. Further investigation with higher resolution imaging and spectroscopy will be needed.
