The galaxy appears to be an elliptical galaxy, exhibiting a smooth and largely featureless morphology. It is characterized by a centrally concentrated luminosity profile, with the light intensity decreasing gradually towards the outer regions. The shape is predominantly round. There is no evidence of spiral arms, dust lanes, or other distinct features typically associated with disk galaxies. The color gradient suggests the presence of an older stellar population, with a yellowish to reddish hue dominating. There is no obvious sign of active star formation. There is no clear evidence of a major ongoing merger. The apparent small size suggests it is a moderately distant object.
