The galaxy presents an overall elliptical morphology, appearing largely smooth in structure. Its color gradient indicates a relatively old stellar population, with a central bulge exhibiting a distinct yellowish hue, likely dominated by older, redder stars. Moving outward from the center, the color transitions to a slightly bluer shade, suggesting the presence of some younger stars, though their contribution appears minor. There may be faint hints of a disk-like component, though it is not sharply defined. The galaxy appears to be relatively isolated, showing little evidence of tidal interactions or recent mergers, though there is potentially a small disturbance in the outer disk on the lower right side. The light distribution is centrally concentrated, consistent with an early-type galaxy or a spiral galaxy seen edge-on, devoid of prominent spiral arms.
