The galaxy presents a generally smooth, elliptical morphology. There are no spiral arms or bar structures discernible within the image's resolution. The light distribution is centrally concentrated, exhibiting a bright core that suggests a relatively high stellar density in the galactic nucleus. Moving outward from the core, the galaxy appears to gradually fade, lacking any distinct, sharp boundaries, with an observed redshift of 0.092521. Subtle color gradients are present, transitioning from a yellowish hue near the core to a bluer tint in the outer regions, which may indicate younger stellar populations present there. The shape is elongated, approaching an intermediate ellipse, without strong evidence of any major disturbances or mergers. Faint irregularities may be present, but they are subtle, suggesting only minor interactions.
