The galaxy appears to be an elliptical or lenticular type. It has a smooth, diffuse appearance with a high degree of central concentration, suggestive of an older stellar population. The galaxy's overall color is yellowish-white, indicating a lack of significant ongoing star formation and a predominance of older, redder stars. There is no discernible spiral arm structure or prominent dust lanes. The shape is elongated, departing noticeably from a perfectly circular morphology. There is no obvious sign of any major tidal disturbance or ongoing merger activity, although a slight asymmetry cannot be entirely ruled out. Based on its appearance, it is likely a relatively massive galaxy with a low star formation rate.
