The galaxy presents a somewhat elliptical morphology. It exhibits a smooth light distribution, with a discernible central bulge but minimal visible structure in terms of spiral arms or prominent dust lanes. The color appears to be predominantly redder, suggestive of an older stellar population and potentially lower levels of ongoing star formation. There is a slight asymmetry in the outer regions, possibly indicating past interactions or minor disturbances. The galaxy appears relatively isolated, with no immediate signs of major mergers or tidal tails. Based on these observations, this galaxy is potentially an elliptical or lenticular galaxy at a moderate redshift. Further spectroscopic analysis would be necessary to confirm the redshift, stellar populations, and star formation rate more accurately.
