The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing a yellow-white hue, indicative of an older stellar population. Moving outward from the center, the galaxy gradually fades, displaying a more diffuse, bluish tinge, potentially indicating some younger stars in the outer regions. There is no distinct spiral arm structure visible. The overall shape is somewhat elongated, suggesting a classification between round and cigar-shaped. There is no apparent major disturbance or clear merging activity observed in this image.
