The galaxy presents a generally smooth morphology, exhibiting a somewhat rounded appearance, although not perfectly circular. The light distribution is centrally concentrated, with a bright yellowish core that gradually fades towards the outer regions. There is faint evidence of some irregular features or minor disturbances in the galaxy's structure, possibly indicating interactions or mergers in its past. These disturbances appear subtle, not significantly disrupting the galaxy's overall smooth appearance. The galaxy's color suggests a population of older stars, with a moderate amount of ongoing star formation indicated by the bluer hues in the less concentrated outer regions. It appears to be a massive galaxy with moderate star formation.
