This galaxy presents an elliptical morphology, exhibiting a high degree of central concentration. The light distribution appears smooth and diffuse, with a notable absence of spiral arms or prominent dust lanes. The color profile indicates a relatively red population, suggesting a dominance of older, lower-mass stars and potentially a lower rate of ongoing star formation. The galaxy exhibits a slight ellipticity, deviating minimally from a perfectly circular shape. There's no evidence of major mergers or significant tidal disturbances in the immediate vicinity, and the overall structure appears undisturbed.