The galaxy presents as a singular, somewhat diffuse object with a smooth, elliptical morphology. The galaxy appears mostly featureless, lacking strong spiral arm structures or prominent dust lanes. There is an observed, centrally concentrated brightness gradient indicating a prominent galactic nucleus. The light profile of the galaxy is relatively symmetric. The overall color appears moderately red, suggesting a stellar population dominated by older, redder stars with little ongoing star formation. The mass of this galaxy is estimated to be very high. There is a second, slightly dimmer, and more diffuse object to the left of the main galaxy. There appears to be no major gravitational disturbances or merging events occurring. The majority of the light originates from the central region, with a gradual falloff in intensity towards the outer edges.
