The galaxy presents an elliptical morphology, appearing moderately elongated. The light profile suggests a centrally concentrated bulge. The color gradient shows a reddish hue concentrated towards the core. The outer regions present a slightly bluer color profile, potentially indicating some low-level ongoing star formation. There is a possibility of minor tidal disturbance visible on one side of the galaxy. There appears to be a secondary smaller galaxy in close proximity that is distinctly bluer in color. This indicates that the galaxy may be undergoing some form of interaction or is in the process of merging.
