The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge. Its overall color is yellowish-orange, potentially indicating an older stellar population and/or significant dust content. There is a very subtle hint of possible disk-like structure, but it does not seem to contain prominent spiral arms. The galaxy's light distribution is fairly concentrated, with a gradual fading towards its edges, suggesting a lack of significant ongoing star formation across the bulk of the galaxy. A slight asymmetry or disturbance in the galaxy's shape could be indicative of a minor gravitational interaction.
