The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular type. The object exhibits a centrally concentrated bulge with a slightly elongated shape, tending towards round, but not perfectly spherical. A subtle disturbance appears within the galaxy's structure which is likely evidence of a tidal interaction or minor merger event. The galaxy exhibits a redder color profile, likely indicating an older stellar population and reduced star formation activity. Overall, the galaxy appears as a massive and relatively quiescent system, but with hints of past or ongoing interactions.
