The galaxy presents a morphology that appears to be transitioning between elliptical and lenticular. The central bulge exhibits a smooth, concentrated light profile, with a color leaning towards the redder end of the spectrum, suggesting an older stellar population. The disk component is subtle but noticeable, displaying a less distinct, diffuse structure surrounding the bulge. There is a slight elongation in the overall shape, deviating from a perfectly spherical form. Evidence of spiral arm structure is absent, pointing away from a typical spiral galaxy classification. The light distribution is generally smooth, without prominent knots or star-forming regions, indicating relatively low star formation activity throughout the galactic body. Based on the image, it appears to be relatively isolated, with no obvious signs of major interactions or mergers with other galaxies.