The galaxy appears as a moderately bright, elliptical-shaped object. The core region exhibits a concentrated luminosity, suggesting a significant density of stars. The galaxy displays a smooth light distribution with no prominent spiral arm structures or patchy star-forming regions readily visible. The object is slightly elongated along one axis, with the ratio of the major to minor axis being approximately 2:1. The color is generally bluish white, indicating the presence of a population of relatively young, hot stars, even though the smooth morphology would be expected of a galaxy with a much older stellar population. There is little evidence of dust lanes or significant gas obscuration within the galaxy from what is visible in this image. Subtle color gradients may exist within the galaxy; however, this would require further spectroscopic analysis.
