The galaxy presents as a relatively smooth, rounded structure, possibly indicative of an elliptical or S0 type. There is a slight elongation, but it is not highly cigar-shaped. The galaxy displays a generally even light distribution, with a concentration of luminosity towards the central region. There is little indication of prominent spiral arms or a well-defined disk. There appears to be some minor asymmetry, possibly caused by a slight tidal disturbance or ongoing minor merger activity, but the overall structure remains largely undisturbed. The light emitted suggests a population of older stars, which is consistent with a relatively low star formation rate.
