The galaxy presents as a smooth, elliptical-like structure. It exhibits a generally reddish-orange hue, suggesting a population of older stars and relatively low ongoing star formation activity. There is no significant visible dust or gas obscuration, and the structure is largely featureless, with no discernable spiral arms or bar. The galaxy appears elongated, potentially cigar-shaped, with a smooth radial gradient in brightness, the core of the galaxy appears to be much brighter and more concentrated than the surrounding regions. There's no apparent tidal disturbance, major merger remnant or interaction with other galaxies.
