The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its overall shape is elongated, exhibiting a cigar-like morphology rather than being perfectly spherical. The light distribution is concentrated towards the center, suggesting a prominent bulge. There is a noticeable colour gradient, with the central region appearing more yellow/red compared to the faint blueish disk, indicative of an older stellar population towards the galactic core. No spiral arm structures or significant dust lanes are immediately apparent, and there are no obvious signs of recent or major merger activity. The galaxy is neither perfectly edge-on nor face-on; it presents an intermediate viewing angle. Overall, the galaxy seems relatively isolated and undisturbed.
