The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, with a gradual decline in luminosity from the core outwards. The central region exhibits a yellow-orange hue, possibly indicating an older stellar population and lower levels of ongoing star formation. Moving towards the outer regions of the galaxy, the color shifts towards a bluer tone, suggesting the presence of some younger, hotter stars, though this effect is subtle. There is no apparent spiral arm structure or distinct features like dust lanes. The overall shape appears close to circular, lacking any obvious elongation or tidal disturbances. Given its smooth appearance and color profile, it is likely an evolved galaxy with a significant fraction of its stellar mass locked in older stars.
