The galaxy exhibits a generally smooth morphology, appearing largely featureless across the observed spectrum. It presents an elliptical-like shape with a high degree of symmetry; the deviation from circularity is subtle, exhibiting an axial ratio close to unity.

The light profile is centrally concentrated, with a bright core that gradually fades into the outer regions. The overall color of the galaxy appears to be slightly redder than the field, suggestive of an older stellar population dominating the light emission. Faint, diffuse emission extends beyond the central region, with some mild variation in color; this could indicate subtle differences in stellar population or dust content within these regions.

There is no clear evidence of spiral arms or a prominent disk structure. A lack of strong blue colors indicates a low rate of ongoing star formation within the galaxy at the time the light was emitted. No tidal features or obvious signs of recent merger activity are apparent.
