The galaxy presents as a single, luminous entity with a slightly irregular morphology. The primary body of the galaxy appears smooth, suggesting an elliptical or lenticular classification, however there are two distinct structures that are visible. The brighter central core exhibits a yellowish-orange hue, indicative of an older stellar population, while another diffuse object is located directly above the main core. The overall distribution of light is fairly concentrated. The galaxy appears to have experienced some disturbances, possibly due to a merger or tidal interaction, with the possible presence of minor tidal tails. The galaxy lacks the spiral arm structure typically observed in spiral galaxies.
