The galaxy exhibits a generally elliptical morphology, appearing elongated with a high degree of cigar shape. A smooth and relatively featureless light profile dominates the overall structure. The central bulge is prominent and displays a bright, concentrated luminosity, suggesting a high stellar density. The galaxy's disk, while present, appears relatively faint and tightly wound. There's very little evidence of prominent spiral arms or distinct features typically associated with active star formation regions. The color gradient suggests an older stellar population, predominantly exhibiting a redder hue. There appear to be no signs of major disturbances in the galaxy's morphology, such as tidal tails or prominent asymmetric features, although there may be a very slight indication of minor disturbances in the outer regions. The galaxy appears to be in a relatively quiescent state regarding star formation activity.
