The galaxy appears to be an elliptical type, with a smooth, centrally concentrated luminosity profile. It has a slightly elongated shape. The galaxy exhibits a yellowish-white color, suggestive of an older stellar population, with some regions of slightly bluer light, possibly indicating regions of on-going, although subdued, star formation. There is no evidence of prominent spiral arms or a well-defined disk structure. The galaxy lacks obvious dust lanes or other signs of significant gas content. Overall, the galaxy presents a picture of a relatively quiescent system with a fairly homogeneous stellar population, based on its shape, color, and surface brightness distribution.
