This galaxy appears to be a lenticular or early-type spiral galaxy, observed at a moderate redshift. The galaxy exhibits a smooth, elliptical light distribution indicative of a dominant bulge component. There is a subtle flattening in the shape, transitioning it from round to a more cigar-like shape, hinting at the presence of a disk, though it is not clearly resolved. The color profile indicates a mature stellar population, with a concentration of light towards the redder end of the spectrum, likely due to older stars within the bulge and disk. There is no evident dust lane, active star forming regions, or bright knots within the galaxy itself, suggesting that it currently has a low star formation rate. No signs of any tidal tails, distortions, or merger events can be observed. The galaxy appears as an undisturbed, isolated system. The physical size of the galaxy appears to be relatively large with a significant stellar mass.
