The galaxy appears to be relatively compact with an overall smooth morphology. The light profile seems concentrated, with a bright central region and a less prominent surrounding halo.

The galaxy exhibits a noticeable color gradient. The core region emits strongly in the green, suggesting active star formation. Surrounding it is an orange region that might be indicative of an older stellar population. There appears to be little evidence of a strong spiral structure. There might be a slight asymmetry in the light distribution that could hint at a possible minor disturbance or interaction. The galaxy's shape is generally elliptical.
