The galaxy presents a smooth, elliptical morphology, exhibiting a notable lack of distinct spiral arm structures. The core region displays a concentrated brightness, suggesting a high stellar density. Progressing outwards from the center, the light gradually diminishes. The overall shape is elongated, reminiscent of a cigar shape. There are no apparent signs of ongoing major merging events or significant tidal disturbances. A subtle red hue is observed in the central region, potentially indicative of an older stellar population.
