The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions into a fainter, diffuse halo. The color is primarily a yellow-orange hue, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes, which further supports the classification as an elliptical galaxy. The galaxy does not appear to be undergoing any major mergers or tidal disturbances, and is relatively isolated. The galaxy is compact and well-defined, with no obvious signs of active star formation in its current state.
