The galaxy appears as a centrally concentrated object with a smooth overall texture. There is no obvious spiral arm structure or distinct features such as bars or rings. The light is dominated by a yellowish hue, suggesting an older stellar population and a possible lack of recent star formation. The galaxy's apparent size is relatively small, and there appears to be a slightly elongated shape to the object; it is not perfectly spherical, hinting at a possible disk component or the early stages of a merger. No tidal tails or signs of ongoing major mergers are visible. The overall morphology points towards a galaxy that may be an elliptical or a lenticular type, with a moderate amount of mass in stars but low specific star formation rate.
