The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a high degree of luminosity, suggestive of a concentrated stellar population. The isophotes appear elongated. The major axis displays a position angle oriented roughly northeast to southwest. The colors suggest a primarily older stellar population, with a relatively low rate of on-going star formation. The galaxy lacks any obvious spiral arm structure or significant dust lanes. There may be signs of a tidal stream or other minor disturbance on the edges of the halo, though this needs further investigation with deeper imaging. Overall, the galaxy is a relatively isolated system without evidence of a major merger.
