The galaxy presents a morphology that leans towards smooth, but also exhibits some features indicative of a disk or disturbance. The overall form is neither perfectly round nor highly elongated, but instead exhibits an intermediate shape. There are no strong indications of a recent major merger, though subtle disturbances and/or a minor interaction may be present. The color profile shows a notable yellow-orange hue within the central region, suggesting an older stellar population. This contrasts with bluer tints observed in what could be outer regions, hinting at possible on-going star formation. The galaxy possesses a moderate estimated size, indicating that it is likely a fairly typical galaxy within the wider population.
