The galaxy appears as a single, centrally concentrated object with a relatively smooth profile. The light distribution suggests a primarily elliptical morphology. The core of the galaxy exhibits a bright, yellowish hue, possibly indicative of an older stellar population dominating the central region. Moving outwards from the core, there's a subtle color gradient to a slightly redder tint in the outer regions. The overall structure appears relatively undisturbed, showing no obvious signs of tidal interactions or major mergers. The shape of the galaxy is nearly circular but appears to be slightly elongated on one axis. There are no visible spiral arm structures or prominent dust lanes, and overall the galaxy appears to have little ongoing star formation.
