The galaxy presents as a generally smooth object, potentially an elliptical or lenticular type. Its overall form is elongated, appearing as a flattened spheroid rather than a perfect circle. The central region exhibits a concentrated brightness, suggesting a prominent galactic nucleus or a dense stellar population. The light distribution appears to fall off gradually from the center, with no distinct spiral arms or other features readily visible. Coloration suggests a population of older stars, with a yellowish to reddish hue dominating the galaxy's light. Based on morphology it does not appear to be undergoing any major merging events or tidal disturbances. The galaxy seems relatively isolated, and the smooth light distribution implies a well-mixed stellar population.
