The galaxy appears to be a relatively compact elliptical or lenticular galaxy with a smooth, centrally concentrated light distribution. The core region exhibits a pronounced yellowish hue, indicative of an older stellar population. Fainter, somewhat reddish extensions are visible, possibly indicating tidal tails or distorted outer regions. The overall shape suggests a spheroid, although there may be some subtle deviations hinting at past or ongoing interactions. There is a clear absence of distinct spiral arms or well-defined dust lanes, consistent with a classification toward the early-type end of the Hubble sequence. The smooth morphology and color gradient suggest a relatively quiescent galaxy with minimal ongoing star formation activity. Faint blue concentrations exist towards the out edges. A likely merger event could be the explanation.
