The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a yellowish-orange core, which suggests an older stellar population and minimal recent star formation activity within the nuclear region. Surrounding the core, there is a slightly fainter, more diffuse halo. The light in this halo region appears to transition to a faint greenish color, possibly indicating a small amount of ongoing star formation, or a difference in the average stellar age in this region compared to the core. The galaxy appears generally elliptical, with a slight deviation from perfect circularity. There is no obvious spiral structure or bar feature visible. No significant tidal disturbances or signs of a major merger event are apparent, though there is the possibility of a minor interaction based on the slight irregularity of the outer halo.
