This galaxy presents as an elliptical morphology, lacking defined spiral arms or a prominent disk structure. The light distribution appears smooth and centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. The core exhibits a yellowish hue, possibly indicative of an older stellar population. The overall shape is elongated, approximating a prolate spheroid. There is no readily apparent evidence of active star formation. There are no indications of tidal features or significant morphological disturbance, suggesting the galaxy is relatively isolated and has not undergone any recent major mergers.
