The galaxy presents a generally elliptical morphology, exhibiting a relatively smooth overall appearance. The central region displays a concentrated luminosity, appearing yellowish-white, potentially indicative of an older stellar population dominating the core. Moving outwards from the core, the color gradually shifts towards a slightly greener hue, possibly suggesting the presence of younger, hotter stars in the outer regions, or variations in dust content. There is no clear evidence of distinct spiral arm structures or a prominent disk. The shape leans towards round, with only slight elongation. No major signs of ongoing mergers or significant tidal disturbances are discernible. Minor disturbances cannot be ruled out, but are not obviously visible.
