The galaxy presents a moderately luminous profile, appearing as a flattened spheroid. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. The surrounding disk, while less prominent, displays hints of a bluer color, potentially indicating regions of more recent star formation. The overall morphology is relatively smooth, with no immediately obvious spiral arm structures or signs of major mergers. Subtle disturbances or minor interactions may be present, but are not clearly defined in this image. The shape is closer to an elliptical galaxy, although there is a slight flattening towards the disc.
