The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated luminosity profile. Its shape is moderately elongated, presenting a slight cigar-like morphology as opposed to a perfectly circular form. The central bulge is characterized by a yellowish hue, suggesting a population of older stars. A faint, extended halo surrounds the central region, with a subtle greenish tinge, potentially indicating the presence of a low level of ongoing star formation, or older stars. There is no obvious indication of spiral arms or significant dust lanes, leading to the conclusion that the galaxy is relatively evolved and quiescent in its star formation activity. There also do not seem to be signs of any major ongoing merger activity.
