The galaxy presents as a somewhat elliptical structure. Its core exhibits a concentrated, bright luminosity, suggestive of a significant stellar population density. The light appears to diminish gradually from the center outwards. The galaxy lacks a defined spiral arm structure, instead showing a smoother, more homogenous distribution of light. There is some evidence of a faint disk, but it appears to be viewed at a shallow angle. The galaxy's halo is faint and extends a moderate distance. There's a slight asymmetry, possibly indicating either minor gravitational disturbance. The galaxy appears to be of moderate size and mass. There is no distinct dust lane or significant signs of active star formation.
