The galaxy presents a somewhat elliptical morphology with a noticeable degree of smoothness in its overall structure. A faint disk-like structure can be tentatively identified, albeit heavily obscured. The galaxy's color profile indicates a population of older stars, as evidenced by the overall reddish and yellowish hues present.

Evidence suggests a possible interaction or recent merger event. The presence of distortions or tidal features would need more detailed study to confirm, but there is a general disturbed appearance to the surrounding region. The galaxy does not appear to be actively forming many stars.
