The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer regions. The morphology is elongated, appearing somewhat cigar-shaped, rather than perfectly circular. A slight blue tinge is present along the edges indicating faint star formation and it is a low star-forming galaxy. There's no strong evidence of significant tidal interactions or major disturbances in its structure. The galaxy appears to be an isolated system, not currently undergoing a major merger. There may be very slight minor disturbances.
