The galaxy presents an overall elliptical morphology, appearing elongated with a high degree of cigar-shapedness. The central region exhibits a brighter, more concentrated luminosity profile, transitioning gradually to a fainter halo or outer envelope. The light distribution suggests a smooth, largely featureless structure, lacking prominent spiral arms or distinct dust lanes. The color gradient shows a redder central region, potentially indicating an older stellar population dominated by evolved stars. Moving outward, the halo appears slightly bluer, possibly signifying the presence of younger stars or ongoing star formation, though the overall star formation rate appears low. There is no clear evidence of major mergers or significant tidal disturbances, though minor irregularities cannot be ruled out. The galaxy appears relatively isolated, showing no strong signs of interaction with nearby companions.
