The galaxy presents a primarily smooth morphology, with a concentrated central bulge. A faint, diffuse disk is suspected, but it is largely featureless. The galaxy exhibits a color gradient, with the central region appearing more yellow-orange, suggesting an older stellar population. The outer regions of the galaxy display a bluer hue, possibly indicating the presence of younger, hotter stars, which are still forming. There is a slight hint of a disturbance in the overall shape, potentially suggesting a minor interaction or past merger event, however, the overall shape is fairly smooth. The galaxy's structure is mostly round. The data suggests it is a moderately massive galaxy with moderate levels of on-going star formation.
