The galaxy presents as a somewhat smooth, disc-shaped structure viewed at an inclined angle. It appears relatively concentrated, with a bright central bulge that dominates the overall luminosity. Fainter, more diffuse regions extend outward from this bright center, suggesting a possible disk. There is no strong evidence of spiral arm structure, but there may be some subtle dust lanes. The galaxy has a yellow-red hue indicating older stellar populations, although blue stars may be present but are difficult to distinguish due to its distance and image quality. The light distribution appears centrally concentrated. The image suggests it is a relatively large galaxy. There is no obvious sign of interaction or a major disturbance and it does not appear to be undergoing a major merger. There seems to be ongoing, but not necessarily intense, star formation.
