The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a concentrated, bright luminosity, suggestive of a high density of stellar population or possibly an active galactic nucleus. The isophotes appear generally regular, indicating a relaxed dynamical state. There is a subtle color gradient present, where the core is a bright yellow, which may indicate an older stellar population. The faint outer regions appear redder than the core, suggesting the potential presence of a more dispersed and somewhat older stellar population. There is no strong evidence of spiral arm structure or significant dust lanes, although at this resolution it would be difficult to identify minor dust lanes. The object shows no obvious signs of recent or ongoing major mergers, although there is very minor disturbance possible near its edges. The galaxy exhibits a moderate redshift. Overall, the galaxy appears to be an elliptical galaxy that is approaching quiescence.
