The galaxy presents as a somewhat elongated, centrally concentrated object. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or distinct star-forming regions. The overall color is consistent with an older stellar population. There is a slight hint of asymmetry to the object, potentially indicating some level of tidal interaction or past merger event, though the bulk of the object appears relatively undisturbed. There may be evidence of a disturbance in the overall shape with possibly some tidal features. The observed morphology suggests that this galaxy may have experienced significant interactions in its past, or is currently undergoing such an event.
