The galaxy presents as a singular, relatively smooth, and elongated structure. It exhibits a color gradient transitioning from a yellower core to slightly bluer outer regions. This is consistent with a likely elliptical morphology, potentially with a disk component. The galaxy appears to have a smaller, rounder companion object in close proximity, suggesting possible interaction or tidal disturbance. There are no prominent spiral arms or distinct features indicative of active star formation on a large scale within the main galaxy body itself. Based on the relative smoothness of the structure, the system likely exhibits a relatively low specific star formation rate.
