The galaxy appears to be a relatively smooth, round object with a bright central bulge that gradually fades into a less luminous halo. There are some very slight blue hues present in the outer regions, but the overall color is somewhat redder, suggesting a population of older stars. There is no obvious spiral structure or distinct features, such as a bar or prominent dust lanes. The galaxy appears undisturbed, showing no signs of a recent major merger or tidal interactions. It seems to be isolated in its environment. The galaxy's morphology is consistent with an elliptical galaxy, though the possibility of it being a face-on spiral galaxy with weak spiral arms can not be entirely ruled out. It would be useful to have more detailed imaging and spectroscopic data to more accurately assess its properties.
