The galaxy presents as a largely featureless object, with a high degree of overall smoothness. It exhibits a generally elliptical morphology, appearing more in-between rounded and elongated than perfectly circular or cigar-shaped. There is a notable concentration of light towards the galactic center, suggesting a prominent bulge or core. The color gradient transitions from a yellow-white core region outwards to a slightly bluer halo, implying a potential decline in the age of the stellar populations with increasing distance from the center. There may be some slight asymmetry or minor disturbances in the outer regions, though they are not dramatically pronounced, and merging is not readily apparent. Overall, the galaxy appears to be a relatively quiescent system, with little evidence of recent major mergers or intense star formation activity, but is clearly forming stars.
