The galaxy presents a generally smooth morphology, with a suggestion of slight asymmetry rather than a well-defined disk structure. Its shape is neither perfectly round nor elongated, appearing somewhat elliptical. There is no strong evidence of spiral arms or a distinct bar. The light distribution is centrally concentrated, with a bright core that fades outwards. A slight bluish tint is visible, primarily toward the center. There are subtle signs of potential minor disturbances or interactions, suggesting a potential recent or ongoing merger event, although a single, dominant nucleus is apparent. Overall, the galaxy appears to be a relatively massive system undergoing moderate levels of star formation.
