The galaxy exhibits a smooth, elliptical morphology with a high degree of central concentration. There is a notable absence of spiral arms or prominent dust lanes. The galaxy's color profile suggests a dominant population of older stars, with a yellowish-red hue concentrated towards the core, potentially indicating a lack of significant ongoing star formation. The light is distributed in a relatively uniform manner throughout the galaxy. It appears to be a relatively isolated galaxy, showing no obvious signs of tidal disruption or interaction with nearby companions and no signs of any active galactic nucleus. The overall shape is elongated, appearing more oval than perfectly spherical.
