The galaxy presents a largely smooth, elliptical morphology with a central, bright nucleus exhibiting a concentrated luminosity profile. The overall color is predominantly yellow-orange, transitioning to a faint green hue on the outer edges, suggesting a possible mix of stellar populations with a dominance of older, redder stars in the core and possible pockets of younger, bluer stars or ionized gas in the outskirts. The light distribution appears relatively even, lacking any prominent spiral arm features or distinct dust lanes. The shape is consistent with a slightly flattened spheroid, with no visible evidence of ongoing major mergers or tidal disturbances, although the possibility of minor interactions cannot be ruled out. The estimated size implies it is a relatively large galaxy. Overall, the galaxy appears to be a relatively massive, passively evolving system.
