The galaxy appears as a centrally concentrated object, with a smooth, unresolved morphology. The core region exhibits a bright, yellowish-white glow that fades gradually toward the outer regions. There's a slight hint of reddish hue on the outskirts. No distinct spiral arms, bars, or prominent dust lanes are visible. The overall shape appears elliptical or lenticular, with no obvious signs of ongoing major mergers or significant tidal disturbances, though faint, minor asymmetric features cannot be entirely ruled out. The light distribution suggests a relatively old stellar population, consistent with low star formation rates.
