The galaxy presents an elliptical morphology, appearing smooth and relatively featureless. It is elongated in shape, displaying a cigar-like structure. The central region exhibits a bright, concentrated luminosity, indicative of a substantial stellar population. Proceeding outward from the core, the luminosity gradually decreases into a fainter halo. There's a subtle color gradient visible, with the central bulge showing a yellowish hue, potentially suggesting an older stellar population, while the outer regions display a slightly bluer tint, hinting at some star formation activity. However, signs of disturbance are minimal; the overall structure appears regular, lacking prominent tidal tails or other indications of recent major mergers, though some minor disturbances can't be ruled out based on this image alone.
