The galaxy presents an elliptical morphology, appearing relatively smooth and spheroidal in shape, with a slight elongation. The central region exhibits a concentrated luminosity gradient, indicating a prominent bulge component likely dominated by older stellar populations. The core of the bulge shows a yellowish-white hue, suggesting the presence of evolved stars. Surrounding the central bulge, there is a less concentrated and bluer colored region, which might indicate more recent star formation in a flattened disk. The apparent overall structure suggests this galaxy could be an early-type spiral, where a relatively large bulge component dominates the galaxy, but there is still a small, flattened disk component that is forming stars. There is no evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy. The galaxy appears relatively isolated and undisturbed.
