The galaxy appears as an elongated, cigar-shaped structure. It exhibits a smooth, featureless morphology with a concentrated central bulge, which transitions into a fainter, extended halo or disk. The color profile suggests a redder core, possibly indicating an older stellar population or significant dust obscuration in the central regions. Moving outwards from the core, there is a gradual shift toward greenish-yellow hues, hinting at the presence of younger stars or lower dust concentrations in the surrounding disk. There is no obvious spiral arm structure or signs of ongoing major mergers or significant tidal disturbances. Overall, the object presents as a relatively undisturbed, evolved galaxy, with a high probability of being an elliptical or lenticular type system.
