The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light profile. The core exhibits a bright, yellowish hue, suggesting a population of older, redder stars. There's little evidence of spiral arm structure or significant dust lanes. The galaxy is mostly smooth with a possible minor disturbance and may be undergoing a merger. The galaxy has a slightly elongated shape, somewhere between round and cigar-shaped. The absence of blue light hints at relatively low levels of recent star formation within the galaxy.
