The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable central bulge. The core region exhibits a concentrated luminosity, suggesting a high stellar density. The galaxy appears to be primarily composed of older stellar populations as indicated by its yellowish-red hue, which is consistent with a lack of significant ongoing star formation. There may be a very faint hint of a disk structure, but the overall morphology is dominated by the spheroidal component. There is no evidence of prominent spiral arms or substantial dust lanes. There are no obvious signs of a major merger event or significant tidal disturbances.
