The galaxy presents as an elliptical morphology, appearing largely smooth and rounded in shape with no obvious spiral arm structures. The light profile is concentrated towards the center, with a gradual decline in luminosity outwards from the core. A small, brighter region can be seen within the central region, which could potentially be due to an active galactic nucleus or increased star formation activity. The color appears primarily yellowish-red, suggesting a population of older stars with little recent star formation. There does not appear to be evidence of any significant ongoing merging events, though there may be some minor tidal disturbance on one side of the galaxy, or simply image artifacts. There is some blue light emission from the spiral arms, indicating that there are some younger stars in the galaxy, albeit relatively few. The overall appearance suggests a mature galaxy with a dominant spheroidal component.
