The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. Its overall shape is largely round, though a slight elongation is perceptible. The core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Moving outward from the center, the color transitions towards a slightly bluer, though still muted, tone. This could indicate the presence of a younger stellar population in the outer regions, albeit less significant than the core. There's no apparent spiral arm structure or significant dust lane obscuration. No significant signs of ongoing or recent merger activity are visible; there are no obvious tidal tails or other morphological disturbances.
