The galaxy appears to be a bright, centrally concentrated object with a noticeable, yet not sharply defined, halo. The core region exhibits a high surface brightness, transitioning to a less intense outer region. Evidence of structure within the main body is subtle, but a slight elongation or distortion can be observed. This suggests a possible interaction or merging event. Some irregular faint spots or clouds are visible in the outer regions. The color profile indicates a relatively bluer central region and a redder extended halo. Based on these characteristics, a classification as an irregular galaxy or a galaxy undergoing tidal disruption is plausible. Additional data, such as spectroscopic information, would be helpful to better constrain the nature of this galaxy.
