The galaxy presents as an elliptical morphology, elongated in shape. The central region displays a high surface brightness, appearing as a concentrated spheroid. Proceeding outwards, the luminosity gradually decreases toward the edges, showing no distinct boundaries. The color gradient appears subtle, but the central bulge seems slightly more yellow compared to the outer regions, which might be slightly bluer, perhaps indicating a difference in stellar populations. The galaxy exhibits no visible spiral arms or prominent dust lanes, suggesting a relatively smooth distribution of stars. There is no indication of a major ongoing merger event, although there is very slight indication of a possible minor interaction. Overall, it appears to be a fairly relaxed and evolved system.
