The galaxy presents as a relatively smooth, somewhat rounded structure. There is some asymmetry in the light distribution, but it is not a strong feature. The central region appears brighter and more concentrated, which is consistent with the presence of a bulge. The galaxy exhibits a primarily yellowish-orange color, with hints of bluer regions on the edges. This color profile suggests a population of older stars with relatively low levels of ongoing star formation. There also seems to be some light emission that could indicate some star formation. There is some indication of minor disturbance in the galaxy shape. This may imply a past or ongoing interaction with another galaxy.
