The galaxy appears to be a single, relatively smooth object with a concentrated central bulge and a faint, extended halo or disk. The central region exhibits a yellowish-orange color, suggesting an older stellar population. The outer regions are more difficult to resolve, but there is a hint of a flattened structure. This suggests a possible disk component. There is no clear evidence of spiral arms or prominent dust lanes within the galaxy. The overall morphology indicates the galaxy is likely an elliptical galaxy with a possible disk structure. There is no strong indication of a major merger event, however there are some minor disturbances visible that could be due to a small interaction. The galaxy has a redshift of 0.327788, indicating that it is relatively far away from us. The overall color indicates that it may be an early-type galaxy with relatively little ongoing star formation, although the presence of a weak blue component may hint at a small amount of star formation.
