The galaxy presents a largely smooth and rounded morphology, with no apparent spiral arms or bar structure. The galaxy exhibits a concentrated luminosity profile, suggesting a significant spheroidal component. The dominant color is a deep yellow, indicative of an older stellar population. There appears to be minimal dust extinction visible. The overall light distribution indicates that the object is not undergoing any major merging events, though there is a possibility of minor disturbances that could be influencing the morphology. The general appearance suggests a relatively passive galaxy with a low star formation rate. The compact size indicates that this galaxy is likely a small, but relatively massive galaxy.
