The galaxy exhibits a largely smooth morphology, with a possible elliptical shape. Its color profile suggests a substantial population of older stars, emitting light primarily in the redder wavelengths. There is a notable absence of strong blue emission, which could indicate a lack of ongoing active star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There is a slight asymmetry, with one side appearing to have a small amount of bluer light, potentially indicating a minor recent interaction or low-level star formation in that region. Overall, the galaxy presents as a passively evolving system.
