The galaxy presents a largely smooth, elliptical morphology. It appears nearly circular in projection, exhibiting a high degree of radial symmetry. A central bulge region is evident, displaying a concentrated luminosity gradient, suggesting a high stellar density. The color profile of the galaxy indicates a redder hue, consistent with a population of older stars and a possible lack of significant ongoing star formation. There are no readily apparent spiral arms or significant dust lanes visible in this image. The galaxy is quite compact in size. There is no evidence of a major ongoing merger event or significant tidal disturbances, though minor distortions can't be ruled out at this resolution.
