The galaxy presents an overall smooth morphology, with a centrally concentrated bulge dominating the light profile. The galaxy exhibits an elliptical shape. The ellipticity indicates a deviation from a perfect circle. Faint disk-like structures may be present within the galaxy, but the resolution is insufficient to clearly resolve them. The galaxy displays a color gradient, transitioning from a bluer hue in the outer regions to a redder hue in the center, suggesting a difference in stellar populations, with older, redder stars being concentrated in the bulge and younger, bluer stars residing in the faint outskirts. The overall color suggests that the galaxy is evolved and dominated by older stellar populations. There is no visible evidence of significant tidal disturbances or ongoing major mergers. Faint features may be indicative of a minor interaction or internal processes.
