The galaxy presents a largely smooth morphology, with minimal evidence of strong spiral arm structure or significant tidal disturbances. It appears to be an elliptical galaxy. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. The core is relatively bright and compact, suggesting a possible active galactic nucleus or a dense stellar population. There is little indication of ongoing major star formation within the galaxy itself, given the lack of distinct blue regions associated with young, hot stars. The overall color is relatively red, consistent with an older stellar population dominated by red giants and low-mass stars. There are no obvious signs of a recent major merger event; the galaxy seems settled and undisturbed. The shape is largely round. Subtle hints of minor irregularities may indicate past interactions or minor accretion events, but these are not prominent.
