The galaxy presents a predominantly smooth, elliptical morphology. Its shape appears elongated, exhibiting a cigar-like form. The galaxy's light distribution is centrally concentrated, with a bright, yellowish core indicative of an older stellar population. There is no discernible spiral arm structure or dust lane features. A faint green coloration is present in the halo surrounding the core. No significant signs of tidal disturbances or mergers are evident. The galaxy appears relatively isolated.
