The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears centrally concentrated, with a gradual decline in luminosity moving outwards from the core. The core region exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outward, the colors shift toward a slightly redder or pinkish tone. There is little evidence of distinct spiral arms or prominent dust lanes. The overall morphology suggests a relatively evolved system. It is likely a massive galaxy with relatively low star formation activity. There is a very slight distortion that may be evidence of a minor disturbance.
