The galaxy appears as a single, relatively smooth object with a somewhat elliptical morphology. It displays a dominant central bulge that emits a bright, yellowish light, suggesting a population of older stars. The color becomes slightly bluer towards the outer regions. There are no clearly defined spiral arms or a prominent disk visible. There is no evidence of any ongoing major mergers, tidal tails, or other significant distortions of the galaxy's shape. The overall light distribution suggests a concentrated stellar population, with the majority of light emanating from the bulge.
