The galaxy presents as a somewhat elongated spheroid. The central region exhibits a concentrated luminosity, with the light appearing significantly more yellow, suggesting an older stellar population dominated by redder stars. This central region smoothly transitions to a less luminous outer halo. The overall light distribution is relatively smooth, displaying no prominent spiral arms or distinct dust lanes. There is a subtle gradient in color from the center outwards, with the outer regions showing a slightly bluer hue, potentially indicating some ongoing star formation, albeit at a low rate. The general morphology points toward an elliptical galaxy with a quiescent star forming history. There is no evidence of any major mergers or tidal disturbances within the limits of the data.
