The galaxy presents a relatively smooth morphology, with a dominant central bulge. The shape appears mostly round. There is evidence of a possible interaction or merger event, with a secondary, less defined structure appearing in close proximity. This secondary structure exhibits a bluer hue compared to the main body of the galaxy, potentially indicating ongoing star formation. The overall color suggests a mix of stellar populations, with the central bulge possibly dominated by older, redder stars, and the outer regions exhibiting signs of younger, bluer stars. There are very slight disturbances in its shape.
