The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high surface brightness, with a concentrated core that dominates the overall luminosity. The light profile appears to gradually fade towards the outer edges, lacking distinct spiral arm structures or significant star-forming regions visible in this image resolution. The galaxy displays a somewhat rounded shape, with a slight deviation towards an elongated form. There is some evidence of a minor asymmetry or disturbance in the galaxy's structure, potentially indicative of a past or ongoing interaction. The overall color of the galaxy leans towards the redder end of the spectrum, suggesting an older stellar population and a relatively low rate of ongoing star formation.
