The galaxy presents an overall elliptical morphology, with a concentrated, bright central bulge. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or distinct disk structures. The core region exhibits a yellowish-orange hue, possibly indicative of an older stellar population. Fainter, diffuse extensions emanate from the central region, blending into the background sky. There is a slight indication of subtle irregularities in the outer regions of the galaxy, potentially suggesting minor tidal disturbances or interactions. There's a hint of bluer emission to one side, indicating possible star formation.
