The galaxy presents as a relatively smooth, elliptical structure. It exhibits a central bulge with a yellowish hue, suggesting an older stellar population. The outer regions appear less defined, gradually fading into the background. There's a slight elongation in its shape, hinting it isn't perfectly spherical. Overall, there are no prominent spiral arms or significant dust lanes visible. The color gradient from the center to the edges suggests a possible decline in star formation activity towards the periphery. There is no evidence of a major merger or significant tidal disturbance.
