The galaxy presents as a relatively compact object, exhibiting a generally smooth morphology with a suggestion of a disk-like structure when using color filtering to highlight its features. The color distribution indicates a range of stellar populations, with a central concentration that exhibits bluer colors, indicative of younger, hotter stars or active star formation. Proceeding outwards to the edges the galaxy turns more red in nature, indicting that this area is more abundant with older stars. There are hints of minor disturbances in the galaxy's form, potentially suggesting past interactions or mergers. No clear spiral arms or a pronounced central bulge are discernible. Overall, the galaxy appears to be in a relatively evolved state, but still displays some features indicating ongoing activity.
