The galaxy presents as a centrally concentrated object with a generally smooth morphology. The color gradient transitions from a yellowish-white core to a slightly redder halo, suggesting a population of older stars more prevalent in the outer regions. The apparent roundness indicates a likely elliptical morphology, although a highly inclined disk cannot be completely ruled out based on this image alone. No distinct spiral arms or bar structures are visible. There is no visual evidence of any major mergers or tidal disturbances. The galaxy displays a consistent and continuous light profile, indicating a lack of significant dust lanes or patches of intense star formation in the visible wavelengths.
