The galaxy appears as a relatively smooth, rounded object. The light distribution is concentrated towards the center, exhibiting a bright central bulge. There is a subtle color gradient, shifting from a warmer, yellower hue at the core to slightly cooler, redder tones towards the periphery. There is little indication of defined spiral arms or significant dust lanes. The overall morphology suggests it may be an elliptical galaxy or a spiral galaxy viewed face-on with a dominant bulge component. Star formation appears to be low within the galaxy. The light suggests an older stellar population is prominent. There may be slight disturbances to its circular shape, with only some indication of minor asymmetry, suggesting a possible past interaction.
