The galaxy appears to be a relatively smooth, centralized object. It exhibits a fairly round morphology, with a bright, concentrated core that graduates outwards into a less defined halo. The color profile suggests a mix of stellar populations. The central region exhibits a yellowish-white hue, which potentially indicates a population of older stars. The outer regions of the galaxy show hints of bluer colors, suggesting the presence of younger, hotter stars and potential ongoing star formation. Overall, the galaxy presents a fairly undisturbed morphology, with no significant signs of ongoing major mergers or tidal disruptions. There may be some minor irregularities in the outer disk.
