The galaxy presents a generally smooth and elliptical morphology. There is a concentrated central bulge that displays a yellowish-orange hue, indicative of an older stellar population. Moving outward from the core, the light gradually fades into a less defined, more diffuse halo. The lack of distinct spiral arms or prominent dust lanes suggests that this galaxy is likely an elliptical galaxy, with a relative absence of ongoing star formation. There is a very slight irregularity in the outer regions which could mean a minor merger event but overall there are no signs of major disturbances or interactions. The galaxy appears to be moderately massive based on the bright and concentrated central luminosity.
