The galaxy presents a largely smooth and centrally concentrated morphology. The light distribution indicates a spheroidal shape, appearing mostly round with some ellipticity. The galaxy's core exhibits a bright, concentrated luminosity, suggesting a dense stellar population or potentially an active galactic nucleus. The color profile transitions from a yellowish-white core to a slightly redder outer halo. This color gradient could indicate an older stellar population in the outer regions of the galaxy. The smooth appearance suggests a lack of significant ongoing star formation across the main body. There is no clear evidence of spiral arms or a prominent disk structure. No signs of major mergers or significant tidal disturbances are apparent.
