The galaxy appears as a centrally concentrated object with a smooth light distribution. The core region exhibits a yellowish hue, potentially indicating an older stellar population. The galaxy lacks any obvious spiral arm structure or distinct features usually associated with disk galaxies. There is a slight blueish tint around the edges of the center, but it is difficult to discern if this is dust or related to a relatively small amount of star formation occurring on the outer parts of this galaxy. The overall shape appears generally elliptical, but there's a slight deviation hinting at a possible interaction or past merger event. There is a faint asymmetrical extension on one side, which may support the minor merger or tidal disturbance hypothesis.
