The galaxy presents as a slightly elongated spheroid, with a smooth, centrally concentrated light distribution. The core region exhibits a distinct yellowish hue, suggestive of an older stellar population and potentially a significant population of dust. Moving outwards from the core, the light fades gradually, with no sharply defined spiral arm structures or prominent star-forming regions discernible in the image. There is a suggestion of a disk-like structure, with a slight flattening visible in the galaxy's overall shape. The absence of clearly defined spiral arms or HII regions indicates a relatively low rate of ongoing star formation within the galaxy. There may be some evidence of minor gravitational interaction with a small object.
