The galaxy presents as a moderately luminous object with a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct central bar. The color profile indicates a higher concentration of redder light towards the core, transitioning to a slightly bluer hue in the outer regions. This color gradient suggests a differential stellar population, with older, redder stars dominating the galactic nucleus and younger, bluer stars populating the outer regions, with some degree of on-going star formation. The overall structure displays a slight elongation, deviating minimally from a perfectly circular shape. Evidence of any major mergers or significant tidal disturbances is absent, although there appears to be a minor asymetry possibly caused by a minor merger. Based on visual analysis, this galaxy is likely a massive system with an estimated stellar mass greater than 10^10 solar masses.
