The galaxy presents as a relatively smooth structure with an elongated, cigar-shaped morphology. The light distribution suggests a centrally concentrated bulge or core, exhibiting a gradual decrease in luminosity moving outward from the center. There is no significant evidence of spiral arm structure or prominent dust lanes, consistent with a classification favoring an elliptical type.

The color profile shows a moderate red shift with light emitted. While seemingly undisturbed, the galaxy appears to be potentially undergoing a minor interaction. Based on the morphology, the galaxy is likely a mature system, suggesting suppressed star formation.
