The galaxy presents as a flattened elliptical morphology, possibly exhibiting a cigar-like shape. Its core is a bright, concentrated yellowish-white, suggesting an older stellar population dominating the central region. The galaxy's color profile shifts towards redder hues in the outer regions compared to the core. The overall smooth light distribution supports a classification toward the elliptical end of the Hubble sequence. The galaxy shows no obvious signs of strong disturbances or interactions, displaying a relatively undisturbed morphology. It displays an unobtrusive halo of light. There is a marginal indication of spiral arms.
