The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of luminosity, appearing nearly spherical. The light tapers off gradually from the core outwards. There is a slight elongation or extension visible towards the left side of the image. This could potentially be the result of minor gravitational interaction. The overall color profile is indicative of an older stellar population, appearing relatively uniform across the galaxy, with a possible slight reddening of the outer regions. The galaxy does not exhibit any prominent spiral arms, or large patches of intense star formation.
