The galaxy presents as an elliptical morphology. It exhibits a smooth, diffuse light distribution, lacking any discernible spiral arm structures or prominent dust lanes. The color appears to be predominantly yellow-orange, suggestive of an older stellar population and lower rates of ongoing star formation within the observed region. The galaxy does not display any strong signs of tidal disturbances or interactions with other galaxies; it seems to be relatively isolated and undisturbed. The round morphology seems relatively normal. The absence of distinct features indicates that the galaxy is not undergoing significant star formation or dynamic processes at the present epoch.
