The galaxy presents as a relatively smooth, centrally concentrated object, likely an early-type galaxy. The galaxy exhibits an overall elliptical shape, with the isophotes appearing mostly round. There may be a very subtle disk-like feature present upon closer inspection, but this feature is very hard to tell. There is no evidence of significant tidal features or major disturbances indicative of recent major merger activity. There may be some slight asymmetries in the outer regions of the galaxy, perhaps suggesting a minor disturbance or recent accretion event. A color gradient is visible, with a yellowish central region transitioning to bluish hues in the outer regions. The yellowish hue may indicate an older stellar population in the center, while the bluer colors may indicate the presence of some younger stars in the outer regions. The overall structure is consistent with a spheroidal stellar distribution, typical of elliptical galaxies. The galaxy appears relatively isolated, without close companions.