The galaxy presents as a relatively smooth, elliptical structure. Its overall shape appears elongated, displaying a cigar-like morphology rather than a circular form. A central bulge is evident, exhibiting a brighter, more concentrated luminosity compared to the outer regions. The galaxy's color profile suggests a dominant population of older stars, indicated by the yellowish-red hues. There are no prominent spiral arms or dust lanes visible, supporting the classification as an elliptical galaxy. No signs of major disturbances or mergers are readily apparent in the image. The galaxy appears relatively isolated and undisturbed.
