The galaxy presents as a single, luminous structure with an overall elliptical morphology, although a distinct asymmetry suggests a potential interaction or merging event. The primary body of the galaxy appears relatively smooth and concentrated, indicating a dominant spheroidal component. A secondary, less prominent luminous region is visible, possibly indicating a smaller galaxy in the process of merging. The color profile appears to be relatively uniform throughout both the primary and secondary regions, with a generally yellow-red hue, suggestive of an older stellar population with lower rates of star formation. Evident disturbance of this galaxy is present; a distinct interaction seems likely.
