The galaxy presents as a moderately bright, elongated object with a generally smooth appearance. Its color profile suggests a slightly higher concentration of older stellar populations, indicated by its subtle reddish-yellow hue and a faint blue coloring towards the edge. The galaxy lacks any obvious spiral arm structure or prominent dust lanes. Its shape is lenticular, with an approximate estimated diameter of roughly 3.7 kpc. There is no evidence of any ongoing major merger activity or significant tidal disturbances; the galaxy appears to be in a relatively quiescent state.
