The galaxy presents as an elliptical system with a smooth, centrally concentrated light profile. The core region appears bright and somewhat diffuse, suggesting an older stellar population with ongoing star formation. There is an absence of well-defined spiral arms or significant dust lanes. The galaxy's shape is elongated, exhibiting an axial ratio of approximately 0.6, with a slight tilt relative to the line of sight. Faint, extended halo components surround the central bulge, but they are relatively indistinct in this image. The overall color index suggests a redder hue, indicative of a population dominated by evolved stars, with the possibility of some contribution from redshift.
