The galaxy presents a predominantly smooth morphology. The light distribution is centrally concentrated, appearing nearly round. There are indications of faint, diffuse features possibly suggestive of disturbances. The color profile suggests a population of older stars, with a concentration of yellow light within the core and redder hues in the faint outer regions. Despite the smoothness, there may be some faint disk-like structure present, or a slight irregularity, indicating a minor merger event in its past or a companion galaxy currently interacting with it. The galaxy appears to have low to moderate ongoing star formation.
