The galaxy appears to be elliptical in shape, displaying a smooth, centrally concentrated light distribution. There is no discernible spiral arm structure or dust lane features, suggesting a relatively old stellar population. The galaxy exhibits a bright, compact core that gradually fades outward. The color is primarily a yellow-orange hue, indicative of older stars and a lack of significant ongoing star formation. There are no signs of tidal tails, strong gravitational lensing, or other indications of recent major merger events. There may be a slight disturbance in its morphology, but it otherwise appears to be isolated and undisturbed.
