The galaxy exhibits a prolate, elongated morphology, appearing cigar-shaped. A brighter, more concentrated central region or core is visible, suggesting a higher density of stellar populations or active galactic nucleus activity. A fainter extension or tidal tail is observed to emanate from the core, possibly indicative of an ongoing or past merger event. The color profile indicates a relatively redder hue. There is evidence of disturbed morphology, possibly related to gravitational interactions or recent mergers. Star formation is likely occurring at a relatively low rate. The galaxy appears to be quite massive.
