The galaxy exhibits an overall elongated, lenticular morphology. The central region appears as a bright, concentrated bulge, characterized by a yellowish-orange hue, likely indicative of an older stellar population. Moving outwards from the core, the disk appears relatively smooth and lacks prominent spiral arm structures. The color shifts towards a slightly bluer tint in the outer regions, possibly suggesting the presence of younger, hotter stars, although star formation is not a dominant feature. There is no obvious presence of dust lanes or significant irregularities in the disk, implying that the galaxy is relatively undisturbed. A minor degree of tidal distortion is a distinct possibilty, given the fuzziness around the edges of the galaxy. The system appears to be in a relatively quiescent state, lacking major starburst activity or active galactic nucleus characteristics.
