The galaxy presents as a centrally concentrated, relatively smooth object. Its overall morphology suggests a spheroid-dominated system, appearing largely elliptical or lenticular. There is a subtle color gradient visible, with a slightly bluer hue in the central regions transitioning to a redder color in the outer parts. This color gradient hints at potential radial variation in stellar populations, potentially due to younger, bluer stars located toward the center and older, redder stars dominating the outskirts. No distinct spiral arms or prominent dust lanes are apparent within the resolution of the image, and there is no indication of any ongoing major mergers or tidal disturbances with another galaxy. The galaxy appears fairly isolated, without any immediately obvious signs of interaction with nearby companions.
