The galaxy appears as a relatively smooth, elongated structure. Its overall shape is elliptical, but deviates slightly toward a cigar-like form. The central region presents a more concentrated, yellowish hue, suggesting a higher density of older stellar populations. The outer regions exhibit a bluer tint, indicative of a small degree of recent star formation activity. There is no visible evidence of a prominent disk structure or spiral arms. No major mergers are apparent, though a minor disturbance might be present. The galaxy shows no sharp edges or distinct features; instead, there is a smooth transition from the bright central bulge outwards to the fainter periphery.
