The galaxy presents as an elongated, cigar-shaped structure, indicative of an elliptical morphology viewed at an oblique angle. The color profile suggests a dominant population of older stars, emitting light skewed towards the redder end of the spectrum. The overall smoothness of the light distribution implies a lack of significant dust lanes or prominent star-forming regions. There is a subtle gradient in color and brightness from the center outwards, with the core appearing slightly more yellow. There is no indication of tidal tails or morphological disturbances, suggesting that the galaxy is relatively undisturbed, with no major mergers in recent history.
