The observed galaxy exhibits a relatively compact morphology, with an elliptical appearance on the plane of observation. There is a possible presence of a central bulge component that is brighter than the surrounding disk. The disk component, although faint, appears to be nearly edge-on. The galaxy displays evidence of possible disturbances or tidal features, suggesting potential ongoing gravitational interactions. This is based on the somewhat irregular shape of the disk. The galaxy's color profile suggests a population of both older and younger stars, potentially due to a recent or ongoing minor merger.
