The galaxy presents a visual morphology suggesting a potential interaction or merger event. It appears to consist of two distinct galactic nuclei embedded within a common, diffuse halo or envelope of stellar material. The upper component exhibits a slightly elongated structure, oriented roughly horizontally within the image frame. The lower component displays a more compact, rounded appearance.

The color distribution across the galaxy is predominantly yellowish-orange, indicative of an older stellar population with relatively low star formation activity. A faint, bluish haze is apparent within the outer regions of the galaxy, particularly in the areas connecting the two nuclei. This may suggest the presence of some younger, hotter stars, perhaps formed as a consequence of tidal forces induced by the interaction.

There are some apparent distortions in the outer isophotes of the galaxy. There may be subtle tidal tails or bridges, connecting it to other objects in the field. The presence of these features supports the hypothesis of an ongoing or recent interaction.
