The galaxy presents as an elliptical morphology, displaying a smooth, centrally concentrated luminosity profile. The major axis of the galaxy is oriented approximately diagonally in the field of view. The color appears bluer in the central region, suggesting the presence of a younger stellar population compared to the redder halo. There are no readily apparent spiral arms or distinct dust lanes visible in the image, consistent with an elliptical classification. The overall appearance suggests a relatively evolved system. There is no major disturbance or merger apparent. There is a slight deviation from perfectly round, towards being cigar shaped.
