The galaxy presents a largely smooth, elliptical morphology. There is a concentration of light in the central region, appearing as a bright, yellowish core, which likely corresponds to an older stellar population. The overall color profile suggests a higher concentration of older stars, indicated by the redder hues in the outer regions, with some bluer stars towards the inner region, perhaps indicating weak ongoing star formation. The shape is generally rounded, trending slightly toward an elongated form, but not significantly cigar-shaped. The galaxy shows no obvious signs of major disturbances or mergers. It appears relatively isolated with no obvious interacting companion galaxies in close proximity.
