The galaxy appears as a relatively smooth, centrally concentrated object with a diffuse halo. The core exhibits a yellowish-white hue, suggesting an older stellar population. There's a subtle color gradient, transitioning to a slightly bluer outer region, hinting at the possibility of ongoing, albeit low, levels of star formation in the galaxy's outskirts. The galaxy's morphology is predominantly elliptical, displaying a high degree of rotational symmetry. There is no evidence of significant tidal disturbances, major mergers, or pronounced spiral arm structures, though a faint, disklike structure may be present. Overall, this galaxy seems to be a fairly isolated system, likely undergoing a phase of quiescent evolution.
