The galaxy presents as a lenticular or possibly an elliptical type, observed at a significant inclination. Its morphology is characterized by a smooth, diffuse light distribution, exhibiting a centrally concentrated bulge.

The color gradient suggests a population of older stars dominating the central region, indicated by the yellow-red hue. Proceeding outward, the light appears bluer, suggesting a higher proportion of younger stars in the galactic disk.

There is a subtle asymmetry to the galaxy's outer edges, but no clear signs of spiral arms or active star formation regions are visible in the image.

The elongation of the galaxy is distinct, implying a non-spherical shape, possibly ellipsoidal. There's no evidence of significant dust lanes or other features that would suggest a recent merger event.
