The galaxy presents a generally smooth and rounded morphology. The central region exhibits a bright, concentrated luminosity, suggesting a substantial stellar population and/or active galactic nucleus. The light appears to be more concentrated in the center, and less dense towards the edge. A slight elongation is visible, but overall, the galaxy appears fairly spheroidal. A patch of redder light is discernible to one side of the main body, possibly indicating a region of dust obscuration, a population of older stars, or a distinct star-forming region. There appears to be no major disturbance or merging activity is observed.