The galaxy presents as an elliptical morphology. The light profile is smooth and concentrated towards the center, indicating a higher density of stars in the core region. The galaxy is elongated, appearing cigar-shaped. There is little evidence of spiral arms or distinct features such as star-forming regions. The color suggests an older stellar population, with a dominant yellowish-red hue. There is no obvious interaction with other galaxies or major disturbances in its structure. The galaxy is fairly massive. Based on the star formation rate, it may be actively forming stars.
