The galaxy appears as a single, relatively smooth structure. The light distribution suggests a mostly elliptical morphology, exhibiting a centrally concentrated luminosity profile. The core region is bright and yellowish-white, potentially indicative of an older stellar population dominating the light output. Faint extensions of the galaxy can be observed, with the primary axis of the galaxy extending towards the lower-left. Overall, the galaxy presents a relaxed, somewhat undisturbed appearance, lacking strong spiral arm features or prominent dust lanes. There is the possibility of an ongoing merger, however, it is much more likely that the structure is simply the product of an older stellar population.