The galaxy presents as a relatively smooth, centralized structure. It exhibits a generally elliptical morphology, appearing mostly round. The core region presents a bright, concentrated luminosity, suggesting a high stellar density. This contrasts with the surrounding halo, which demonstrates a gradual decrease in light intensity.

There is some indication of tidal disturbance, particularly a small extended feature towards the lower edge, potentially indicative of minor interaction with another galactic object or past merger event. Overall color indices suggest a evolved stellar population. There's a noticeable lack of prominent spiral arm structures or active star-forming regions within the observed wavelength range.
