The galaxy appears to be a single, luminous entity with a predominantly smooth morphology. Its overall shape is relatively round, showing a slight deviation toward an elliptical form. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population.

A faint disk structure may be present, as evidenced by the slight flattening along one axis. There appears to be very faint spiral arms visible in the galaxy. There is a notable absence of significant dust lanes or prominent star-forming regions, suggesting a lower rate of recent star formation. No strong evidence of a major merger event is apparent, although there is a presence of a nearby object in the image, suggesting possible minor gravitational interaction.
