The galaxy presents a predominantly elliptical morphology, viewed nearly edge-on. The central bulge appears smooth and concentrated, exhibiting a yellowish-orange hue, suggestive of an older stellar population. There is a faint, diffuse disk component, extending along the major axis. No distinct spiral arm structures are discernible. The overall color profile indicates relatively low levels of ongoing star formation. There is no obvious indication of a recent or ongoing major merger event or significant tidal disturbance; however, low-level merger features are subtle. The galaxy appears relatively isolated.
