The galaxy presents as a centrally concentrated, relatively smooth object with an overall elliptical morphology. A bright, compact core region dominates the galaxy's luminosity profile, exhibiting a slightly reddish tint compared to the surrounding disk. Fainter, bluer material appears to populate the outer regions of the galaxy, suggesting the presence of some degree of ongoing, albeit low-level, star formation. There is no strong evidence of spiral arm structures or a prominent disk, consistent with a galaxy tending towards an early-type classification. There are no obvious signs of significant tidal disturbances or recent merger activity, with the overall structure appearing relatively relaxed and undisturbed. The galaxy's apparent color is intermediate, indicating a mixed stellar population with both older, redder stars and a younger, bluer component.
