The galaxy exhibits a morphology that is neither purely elliptical nor a well-defined spiral. It presents a somewhat rounded overall structure, with a noticeable concentration of light towards the central region, suggesting a bulge. However, the light distribution isn't perfectly smooth; it shows some irregular features and lumps that indicate possible disturbances. The galaxy appears to have a few bright, concentrated areas, possibly star-forming regions or the nuclei of merging galaxies. There also appears to be a light tidal tail extending off of the galaxy. Color variations are subtle, showing a generally yellowish-orange hue, with the bright concentrations being slightly more reddish. This potentially signifies older stellar populations, although the redder areas could also indicate regions obscured by dust. A slight asymmetry in the outer regions is also observed, suggestive of tidal interactions or a recent merger event, which appears to be ongoing. 
