The galaxy appears as a relatively smooth, elongated structure. The light distribution seems concentrated towards the center, suggesting a prominent bulge. The color is generally yellowish-white, with a slightly redder hue in the central region and some faint bluish tones toward the edges. This color gradient may indicate a population of older stars in the bulge and relatively younger stars within a developing disk. No spiral arms are clearly discernible. Based on its shape and morphology, this galaxy is likely a lenticular or early-type spiral galaxy seen at an oblique angle. There are no apparent signs of major interactions or mergers with other galaxies, although there may be some subtle disturbances in its outer regions. The object's morphology is consistent with a quiescent or passively evolving system with a moderate mass and low star formation rate.
