The galaxy presents a lenticular, or possibly elliptical, morphology. The primary color is a reddish-yellow hue concentrated towards the galactic center, which suggests an older stellar population dominating the core. The outskirts exhibit a fading, bluish-green tint, possibly indicating the presence of younger, hotter stars, though this is much less prominent. The galaxy's shape is elongated, appearing cigar-shaped, with a smooth, diffuse profile. There are no distinct spiral arm structures or prominent dust lanes visible. The overall impression is of a relatively evolved system, potentially undergoing relatively low levels of star formation activity. There is no obvious evidence of recent or ongoing major merger events or significant tidal disturbances.
