The galaxy presents as an elliptical morphology, elongated in shape with a cigar-like appearance. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. The color profile indicates a likely evolved stellar population, with a yellowish-red hue dominating the central regions. The outer regions of the galaxy fade gradually, showing a smoother distribution of light. There is no readily apparent evidence of distinct spiral arm structures or significant dust lanes within the galaxy's disk, which supports the classification as an elliptical galaxy. The lack of strong blue light suggests relatively low ongoing star formation rates. Some minor asymmetrical light distribution is observed.
