The galaxy presents as a smooth, centrally concentrated object with a notable bulge. It is elongated in shape, approaching a cigar-like morphology. The central region exhibits a yellowish hue, indicative of an older stellar population, while the outer regions show a hint of blue, suggesting the presence of some younger, hotter stars, albeit at a lower proportion. There are no readily apparent spiral arm structures or significant dust lanes visible. No signs of major ongoing mergers are immediately clear, although there are subtle disturbances. Overall, the galaxy appears to be an elliptical galaxy, with a slight amount of active star formation in the outer regions.
