The galaxy presents as a somewhat elliptical or possibly disk-like structure, though its roundness is not immediately apparent. It exhibits a relatively smooth appearance overall, with a concentrated central bulge region characterized by a yellowish-gold hue. This color likely indicates an older stellar population within the bulge. There is some evidence of a fainter, less defined disk component extending outwards from the central region. The galaxy appears to be undergoing a relatively low rate of star formation, given the lack of prominent blue regions associated with young, hot stars. There is no strong morphological disturbance or sign of recent major merger activity, although the possibility of minor interactions or disturbances cannot be ruled out based on this image alone.
