The galaxy appears to be in a state of merging or interaction. There is a larger, more diffuse central component displaying a yellowish hue. The morphology of this component is difficult to categorize with certainty, but it may be considered elliptical or lenticular due to its smooth appearance and lack of distinct spiral arms.

A secondary, smaller component is visible to one side of the main body. It is more compact and displays a bluer color. This suggests a potentially younger stellar population within this secondary component, perhaps indicative of ongoing star formation triggered by the interaction.

The overall shape of the system is somewhat irregular and elongated, rather than a simple, symmetrical form, further supporting the hypothesis of a merging event. Evidence of tidal tails or bridges is not immediately apparent, but the distorted shape suggests gravitational disturbance.
