The galaxy presents a somewhat amorphous morphology, appearing as a system undergoing a possible interaction or merger event. The central region exhibits a concentrated, bright yellowish-white core, suggesting an older stellar population or a dust-obscured active galactic nucleus. A fainter, more diffuse extension projects from this central region.

The main body displays intermediate ellipticity, tending towards a more spheroidal shape, but with discernible irregularities. There is evidence of possible tidal features or disrupted arms extending outwards. The overall color profile is dominated by warmer hues, especially in the core, with a bluer tint detectable in the peripheral regions.

The galaxy's structural irregularity and disturbed morphology is indicative of a potentially ongoing or recent gravitational interaction, perhaps a minor merger. The presence of both older, redder stellar populations in the core and younger, bluer populations in the outskirts is consistent with a scenario of triggered star formation. The estimated size is a few kiloparsecs in radius.
