This galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy. It exhibits a dominant bulge with a concentrated central region that transitions gradually into a fainter, elongated disk. The color profile suggests an older stellar population, likely dominated by redder stars, concentrated in the bulge and inner disk. The shape is somewhat elongated, with a ratio of major to minor axes of approximately 3:1, indicating a moderate degree of flattening. There's a subtle hint of a possible disk structure, but no distinct spiral arms are discernible. The overall morphology suggests a system undergoing, or having undergone, a significant decline in star formation. There's little to no evidence of recent major merger activity or significant tidal disturbances in the immediate vicinity. The galaxy has an estimated size of approximately 8.5 kpc.
