The galaxy presents as a somewhat diffuse object with an elliptical morphology. The core region exhibits a concentrated luminosity, appearing distinctly yellow, which may indicate a population of older stars. There's a subtle color gradient extending outward from the core, with the outer regions appearing slightly bluer, hinting at the presence of some younger stellar populations, albeit less prominent than in the core. The edges of the galaxy lack a sharp definition, blending gradually into the background sky. Subtle, disturbed features can be seen in the disc, showing a possibility of past or current gravitational interaction. Overall, the galaxy appears to be a moderately massive system with ongoing, but relatively low, star formation activity.
