The galaxy presents an apparent morphology indicative of a system undergoing tidal interaction. The primary galaxy exhibits a relatively smooth light distribution, with a core of higher intensity. It appears somewhat elongated in shape, transitioning from a near-spherical form to a more cigar-shaped appearance.

A secondary object, likely a dwarf galaxy or a tidal feature resulting from a galaxy merger, is situated nearby. A faint bridge of light, potentially composed of stars and gas stripped from the galaxies during their interaction, connects the two.

The galaxy colors indicate a presence of both older stellar populations, inferred from the redder hues, and younger, bluer stellar populations. This blend of stellar ages implies an ongoing or recent star formation event.

The overall impression is one of a dynamically disturbed system, possibly in the late stages of a minor merger or a close encounter. The lack of clear spiral arm structure in the primary galaxy further suggests a history of gravitational interactions.
