This galaxy presents as a single, luminous object with a generally smooth morphology. It is nearly circular in appearance, exhibiting a high degree of central concentration. The galaxy is noticeably brighter in its core, gradually fading towards the edges. There is a general lack of distinct features, spiral arms or prominent dust lanes. However, there is a slight asymmetry that could indicate some minor gravitational disturbance or interaction. No merger seems apparent from the observation. The light suggests a population of old stars.
