The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, exhibiting a gradual radial decline in luminosity from the core outwards. The core region displays a bright, yellowish hue, suggestive of an older stellar population. The outer regions are fainter, and the transition between the core and the outer halo appears continuous. There is a slight elongation visible, but the overall shape is primarily spheroid. There are no apparent spiral arm structures, dust lanes, or strong tidal features detected. There appears to be some minor disturbances, potentially due to a small merger occurring. The color profile shows a redder core and a gradual blueing towards the outer parts of the galaxy.
