The galaxy presents as a relatively compact object, appearing nearly spheroidal in overall morphology. Its light distribution appears somewhat centrally concentrated with a bright, possibly unresolved core region. The galaxy exhibits a noticeable blue hue overall, suggestive of a relatively young stellar population or ongoing star formation within its structure. Some subtle, irregular features are observed along the outer edges. There is a slight distortion or a faint extension visible, giving an indication of possible gravitational interaction or recent minor merger activity. This interaction may contribute to the presence of disturbed regions and irregular shapes. Overall, the galaxy appears to be a luminous, active system with possible signs of tidal disruption.
