The galaxy presents a generally smooth morphology. It appears elliptical in shape, though not perfectly spherical, trending slightly towards a more elongated, but not cigar-shaped, form. There is no strong evidence of a disk component or spiral arms, with only subtle deviations in surface brightness. The color profile suggests a population of older stars, exhibiting a reddish-yellow hue. There is minimal evidence of ongoing major star formation. No obvious signs of recent or ongoing merger activity are detected, although a slight asymmetry could indicate past minor interactions. The galaxy appears to be relatively undisturbed.
