The galaxy presents as a slightly elongated, elliptical structure with a noticeable central bulge. Its color appears to be yellowish-white in the central region, indicative of an older stellar population. Fainter, bluish hues are visible in the outer regions, potentially suggesting the presence of some younger, hotter stars or ongoing star formation at the periphery. There appears to be a smooth transition in luminosity from the center outwards, with no obvious spiral arm structures or prominent dust lanes. The galaxy exhibits a relatively high degree of central concentration with a gradual fade towards the edges, characteristic of an early-type galaxy at a moderate redshift.
