The galaxy presents as a relatively smooth, elliptical structure. The light distribution is concentrated towards the center, exhibiting a bulge-dominated morphology. There is an apparent lack of distinct spiral arms or features typically associated with disk galaxies. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated along its major axis. The color profile is relatively uniform, with a slight shift towards redder hues, suggesting an older stellar population and potentially lower levels of ongoing star formation. Faint extensions or tidal features are not readily apparent, suggesting it is not currently undergoing a major merger event.
