The galaxy exhibits a roughly elliptical morphology. The central region displays a concentrated, luminous core, appearing smooth and possessing an orange-red hue, indicative of an older stellar population. Extending outward from the core, a less defined, fainter halo is observed with hints of a more bluish color, suggesting the presence of some younger stars. There is a noticeable asymmetry in the galaxy's outer structure, with a slightly extended feature visible on one side, possibly a tidal tail or a disturbance due to an interaction. Overall, the galaxy appears to be in the process of merging, showing a mix of smooth features and subtle disruptions. The galaxy is fairly massive and has very little star formation.
