The galaxy presents as an elliptical morphology, exhibiting a generally smooth structure without readily discernible spiral arms or significant substructure in this image. Its shape is more in between round and cigar shaped than completely circular. The galaxy's color profile suggests a relatively evolved stellar population, with a more pronounced concentration of light towards the red end of the spectrum. This implies older stars are the dominant population. There is a slight visual indication of a disk-like feature or subtle flattening. There is no strong evidence for ongoing major merger activity or significant tidal disturbances in the galaxy's morphology. Any features might be minor and within the galaxy's main body.
