The galaxy presents as a relatively smooth, elongated structure. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. Proceeding outward from the core, the luminosity gradually diminishes into a fainter, more diffuse halo. There is a slight color gradient moving outwards from the center, with the core appearing more yellow/white, and the edges exhibiting a more blueish hue. This color gradient could indicate a change in stellar population age, with older stars concentrated in the center and younger stars in the outer disk. Although mostly smooth, there is faint evidence of some features indicative of a disc structure, but at an angle making them difficult to discern. There is no visual evidence of recent major mergers or significant tidal disturbances, however, there might be minor disturbances within the galaxy. The overall morphology suggests a galaxy undergoing a relatively quiescent period of star formation.
