The galaxy presents an elliptical morphology, with a relatively smooth appearance. The galaxy exhibits a concentrated central bulge, surrounded by a more diffuse halo. The color profile suggests a slightly redder central region compared to the outer regions, potentially indicating an older stellar population in the bulge. There is little evidence of spiral arms or significant star formation regions within this galaxy. The overall structure appears undisturbed, suggesting a lack of recent major mergers or interactions. There might be a very faint disk surrounding it.
