The galaxy presents a largely elliptical morphology, exhibiting a high degree of central concentration. The central bulge is a prominent feature, displaying a smooth, yellowish-white luminosity profile, suggestive of an older stellar population dominating this region. Moving outwards from the core, the galaxy exhibits a more diffuse structure, with colors gradually shifting toward redder hues. There is very little evidence of spiral arm structures or significant dust lanes, which contributes to its generally smooth appearance. Faint indications of tidal features are noticeable, potentially hinting at past or ongoing minor gravitational interactions with other galaxies. Overall, the galaxy appears to be a relatively massive, evolved system, potentially undergoing relatively low levels of star formation.
