The galaxy appears as a centrally concentrated, elliptical structure. Its light profile suggests a relatively smooth distribution, lacking prominent spiral arms or a distinct bar feature. There is a clear color gradient visible, with the central region exhibiting a strong yellowish-orange hue, suggestive of an older stellar population dominated by red giant stars. Moving outwards from the core, the galaxy gradually transitions to a redder color, indicating a decrease in the mean stellar age and potentially, increased metallicity in the inner regions. There are no obvious signs of ongoing or recent major mergers or significant tidal disturbances in its morphology. The morphology is fairly well-rounded, though not perfectly circular, with only the slightest suggestion of elongation. The overall appearance is indicative of a relatively massive galaxy, likely in the later stages of its evolution, with a relatively low star formation rate.
