The galaxy presents a generally smooth, elliptical morphology. It is nearly circular in appearance, with little evidence of a distinct disk structure. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar population density. The overall color profile leans towards redder wavelengths, hinting at an older stellar population and/or significant dust content. There are no immediately obvious signs of major mergers or significant tidal disturbances. Subtle irregularities are present, but they do not dominate the overall structure.
