The galaxy presents as a moderately luminous object with an elongated, cigar-shaped morphology. The core region exhibits a concentrated, smooth distribution of light, appearing yellow-white in color, suggesting a population of older stars. Moving outward from the central bulge, the galaxy shows a gradual decrease in surface brightness. Faint hints of what might be a disk-like structure are visible, extending along the major axis, although it appears relatively featureless and disturbed, with no distinct spiral arms apparent. The color shifts subtly toward redder hues in the outer regions, indicating potentially older stellar populations or increased dust extinction. There are possible signs of a minor disturbance or interaction in the form of an asymmetry in the light distribution; overall it appears mostly undisturbed with a small chance of having been part of a minor merger in the past.
