The galaxy presents as a diffuse, elliptical structure. Its central region exhibits a concentrated luminosity, suggesting a higher density of stellar populations or possibly an active galactic nucleus. The overall color gradient transitions from a yellowish-orange core to a fainter, bluish halo. The elongation of the galaxy indicates a deviation from perfect sphericity, with a suggestion of a cigar-like shape. There are subtle hints of minor disturbances in the galaxy's structure, possibly indicative of past or ongoing interactions. The lack of well-defined spiral arms or prominent dust lanes suggests a relatively smooth morphology.
