The galaxy presents as an elliptical morphology, appearing smooth and relatively featureless. Its shape tends towards a cigar-shaped or elongated form. The central bulge region exhibits a bright, concentrated luminosity, likely indicative of a high density of stars. A disk component is present, though less prominent, with a bluer color compared to the bulge, suggestive of ongoing or recent star formation activity. There appears to be no strong indication of a major merger event in its recent history, although a faint asymmetry may hint at minor tidal disturbance or interaction. The galaxy is a relatively massive system with a moderate rate of star formation.
