The galaxy presents a smooth, elliptical morphology, with a notable lack of distinct spiral arms or prominent features. Its overall shape is elongated, resembling a cigar, but with rounded edges rather than sharp points. The central region appears brighter and more concentrated than the outer edges, showing a gradual decrease in luminosity from the core outwards. The color profile suggests a population of older stars, as it leans toward redder hues rather than the blue tones associated with active star formation regions. There is no visual evidence of ongoing merging activity or major disturbances in the galaxy's structure. The galaxy's smooth appearance and lack of features indicate it is likely a relatively evolved system.
