The galaxy presents as a resolved object with a notable color gradient. The central region exhibits a concentrated, smooth morphology, and a reddish-yellow hue, suggestive of an older stellar population, or possibly the presence of dust. Extending outward, the galaxy displays a bluer component, less concentrated and more diffuse. This bluer region may be indicative of ongoing star formation. There is some evidence of disturbed morphology suggesting either internal dynamics or possible interactions with another galaxy but this is ambiguous. The galaxy exhibits a somewhat spheroidal overall form, though not perfectly circular.
