The galaxy presents a relatively smooth, elliptical morphology with a discernible core. The core exhibits a concentrated luminosity, suggesting a high stellar density or potentially an active galactic nucleus, although no distinct jet or accretion disk is readily visible in this image.

A subtle color gradient is observed, transitioning from a yellowish-white hue in the central region to a bluish tint in the outer portions. This may indicate a change in the stellar population, with older, redder stars dominating the core and younger, bluer stars located more peripherally. It could also reflect the presence of dust lanes absorbing blue light in the inner regions.

There is evidence of minor disturbances in the outer structure, possibly indicative of a past or ongoing interaction or merger event. These disturbances are subtle, and the overall structure retains its primarily elliptical form. No strong spiral arm structures are present. The galaxy appears to be in an intermediate stage of evolution, not fully settled but not undergoing a dramatic transformation.
