The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, indicative of an older stellar population. The galaxy appears to be relatively undisturbed, with no signs of major mergers or significant tidal features. A faint, slightly bluer region is discernible towards the lower portion of the galaxy, possibly suggestive of localized star formation activity or a subtle disk-like component. The galaxy's overall shape is moderately rounded, deviating slightly from a perfectly circular form, with a hint of elongation. Overall, the galaxy exhibits characteristics consistent with a relatively massive system, with a subdued star formation rate.
