The galaxy presents a generally smooth morphology. It appears to be elliptical, with an overall round shape. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy exhibits a concentrated central bulge, with a gradual decrease in luminosity extending outwards. The color profile suggests a population of older stars, contributing to the yellow and red hues. There is no obvious indication of active star formation regions or significant dust lanes. The overall structure appears undisturbed, with no major tidal features or signs of ongoing merging activity. There are no major distortions in its shape. The light profile indicates it is a massive system. 
