The galaxy appears as a moderately bright, elliptical structure. Its core region exhibits a concentrated, yellowish-white glow, suggesting a higher density of older stellar populations. The overall color gradient shifts towards a redder hue in the outer regions, indicating a potential decrease in younger, bluer stars and an increase in dust absorption further from the center. The galaxy has a relatively smooth appearance, with no readily apparent spiral arm structures or prominent dust lanes visible in this image. A slight elongation is observed, giving it a somewhat cigar-shaped appearance. There is no immediately obvious evidence of major merger activity or significant tidal disturbances. The galaxy's morphology appears to be that of a relatively undisturbed, evolved system.
