The galaxy presents as a relatively compact and luminous object. It exhibits a primarily smooth morphology, with a roughly elliptical shape but some irregularities. The galaxy's light is dominated by redder wavelengths, with a noticeable contribution from green, suggesting a stellar population of intermediate age. The core of the galaxy appears very bright and is surrounded by a more diffuse halo. There is some evidence of minor disturbances, possibly hinting at interactions, but the galaxy does not appear to be undergoing a major merger. Overall, it appears to be a massive, relatively evolved galaxy with a modest level of ongoing star formation.
