The galaxy appears to be an elliptical galaxy, displaying a smooth, relatively featureless morphology. It exhibits a concentrated central bulge that dominates the overall luminosity, with the light gradually fading toward the outer regions. The galaxy's shape appears generally round. There is no indication of distinct spiral arms, a bar structure, or signs of significant dust lanes. The galaxy does not appear to be undergoing any major merging activity. There is a possible slight disturbance, but it is unlikely to be a significant merger event. The galaxy presents a yellowish-white hue, indicative of an older stellar population with a low star formation rate.
