The galaxy presents as an elliptical morphology, with a smooth, featureless light distribution. It appears elongated, but not highly so, suggesting a moderate ellipticity. The color gradient is subtle, with a slightly bluer hue in the central region transitioning to a redder color toward the outer edges. This may indicate recent star formation occurring within the core. There is no obvious evidence of spiral arms, bars, or other distinct structural components. The overall appearance suggests a relatively evolved system, potentially with a substantial population of older stars. No tidal features or distortions are visible, suggesting it is not currently undergoing a major merger or interaction, though there may be evidence of minor disturbances in the structure. The galaxy exhibits a strong concentration of light toward the center, indicating the likely presence of a dense central bulge.
