The galaxy presents a generally smooth, elliptical morphology with a somewhat elongated shape. Its core is a bright, concentrated region exhibiting a yellowish-white hue, indicating an older stellar population. Progressing outwards from the core, the galaxy's luminosity gradually decreases. Faint, diffuse extensions are visible surrounding the central body. These extensions appear slightly irregular and contain hints of bluish tones, which could indicate regions of ongoing or recent star formation. The overall structure lacks distinct features, such as spiral arms, and it does not appear to be undergoing a major merger. There may be evidence of minor disturbances in the outskirts, perhaps hinting at past interactions or accretion events, but the dominant impression is that of a relaxed, relatively evolved system.
