The galaxy presents as an elongated, cigar-shaped structure. A notable feature is a brighter, more concentrated region located towards one end of its major axis. The overall color profile suggests the presence of evolved stellar populations, likely dominated by older stars, with a yellowish-red hue. Some bluish coloring is detected in the outer regions of the galaxy. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy shows signs of possible gravitational disturbance or interaction; it is likely in the late stages of merging with another galaxy.
