The galaxy appears to be a relatively smooth, elliptical type. The light distribution is centrally concentrated, with a noticeable decrease in intensity moving outwards from the core. It has a slightly elongated shape, appearing to be between round and cigar-shaped. There is a subtle color gradient, with the central region exhibiting a yellowish hue, potentially indicating an older stellar population. No strong spiral arm features or significant dust lanes are visible. The galaxy exhibits no obvious signs of major merging activity or strong tidal disturbances.
