The galaxy presents as a relatively smooth, elliptical object. Its central region exhibits a bright, concentrated luminosity, suggesting a high density of stars, possibly an older stellar population. The galaxy appears to be a flattened spheroid; the lack of clearly defined spiral arms or significant dust lanes contributes to the overall impression of a well-mixed stellar population. There may be some indication of a slight disturbance or asymmetry in the outer regions but otherwise the morphology shows a lack of significant morphological disturbances, hints of ongoing or recent major mergers or substantial star formation activity. The galaxy's color is generally yellow, indicating a higher proportion of older, cooler stars relative to hotter, younger, blue stars. Overall, the galaxy appears to be a fairly massive, relatively quiescent elliptical galaxy, consistent with a high mass, low star formation rate, and large size.
