The galaxy appears as a relatively compact and smooth object. It exhibits a roughly elliptical morphology with a bright, concentrated central region, likely indicating a prominent bulge or core. The color profile suggests a generally older stellar population. The overall structure is largely featureless, with no obvious spiral arms or significant dust lanes visible. There is a faint blue tint that might indicate low levels of recent star formation. I observe a smooth transition in luminosity from the center outwards. The galaxy's roundness indicates that it is not observed edge-on. There is no evidence of major ongoing mergers, though there are subtle disturbances.
