The galaxy presents as a centrally concentrated object, displaying a largely smooth morphology. It exhibits an elliptical shape, appearing elongated but not excessively so. The color profile indicates a dominant population of older stars, particularly in the central bulge, which shows a strong orange-red hue. The outer regions of the galaxy exhibit a faint blue tint, suggesting the presence of a younger, though likely less significant, stellar population. There is no readily apparent spiral structure or dust lanes. It appears relatively isolated, without any obvious signs of recent or ongoing major merger activity, although some minor disturbances cannot be ruled out. The galaxy appears to be relatively massive and actively forming stars.
