The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It exhibits a moderately elliptical shape. A faint, diffuse halo surrounds the brighter central region, indicating a gradual decline in luminosity with increasing distance from the galactic center. There is no obvious spiral arm structure or prominent dust lanes visible in this image, suggesting that it could be an elliptical or lenticular galaxy. Close inspection shows no sign of recent or ongoing major merging events, although slight asymmetry suggests the possibility of a past minor interaction or disturbance. The core region appears yellowish-red, which could indicate a population of older stars with low star formation activity. The extended halo has a bluer hue, possibly due to younger stars.
