The galaxy presents as an elongated, cigar-shaped structure. It appears relatively smooth in texture, lacking defined spiral arms or prominent dust lanes. The core region seems to exhibit a higher concentration of luminosity. The color profile suggests the presence of an older stellar population, as it shows redder light. Faint traces of possible disturbance, such as slight irregularities in the outer halo, could hint at minor gravitational interaction or past merger events. However, the primary morphology indicates a system dominated by a bulge-like structure.
