The galaxy presents as a slightly elliptical object with a concentrated central bulge. The core exhibits a yellowish hue, suggesting an older stellar population. A subtle disk is present surrounding the bulge. The disk exhibits a bluish tint in some portions, implying the presence of younger, hotter stars, or star forming regions. The disk appears somewhat distorted or disturbed, possibly indicating a past or ongoing minor interaction or merger event. Overall the galaxy appears to be relatively massive with a moderate amount of star formation activity.
