The galaxy appears to be an elliptical or lenticular type, with a smooth, concentrated central bulge. There is a noticeable lack of distinct spiral arms or dust lanes. The overall shape is approximately round, though there is a slight elongation present. The color gradient suggests a population of older stars, with a yellowish hue dominating the central region, fading to redder tones in the outskirts. There is a suggestion of minor tidal disturbance, possibly indicating a past or ongoing interaction with another galaxy, or internal activity.
