The galaxy presents as a primarily smooth, elliptical morphology. The central bulge exhibits a concentrated, reddish hue suggesting an older stellar population. Surrounding the bulge, a fainter, bluer disk-like structure is subtly discernible, indicating the presence of a younger stellar population and ongoing, though potentially low, star formation activity. The overall shape is elongated, leaning towards a cigar-shaped appearance. No significant signs of major disturbances or mergers are readily apparent, though subtle asymmetries might suggest minor gravitational interactions or past disturbances. The galaxy appears relatively isolated, which aligns with a lack of major merger signatures.
