The galaxy presents as a relatively smooth, elliptical morphology with a slight elongation. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the galactic center. The color profile indicates a dominant population of older stars, evidenced by the yellowish hue, with limited indications of active star formation. The outer regions of the galaxy are less defined, gradually fading into the background sky, indicating a lack of prominent spiral arms or significant dust lanes. There is no apparent ongoing merging activity or major disturbances in its structure. Overall, this galaxy appears to be a mature, quiescent system with a relatively simple structure.
