The galaxy exhibits a notable degree of structural disturbance, suggestive of an ongoing or recent interaction. The overall morphology appears to be neither purely elliptical nor a well-defined spiral, possessing characteristics of both. The core region displays a smooth, centrally concentrated light profile. Fainter, diffuse features extend outwards, exhibiting an irregular shape. There are some features that suggest possible tidal tails or disrupted arm structures. The color profile of the galaxy suggests a relatively old stellar population, with a noticeable redder hue in the central regions. The bluer components are located in a some of the outer regions and likely mark regions of more recent star formation. Dust lanes are not apparent, and there is no clear evidence of a strong bar structure.
