The galaxy presents as a fairly elliptical, somewhat elongated structure with a smooth and diffuse light distribution. There is a centrally concentrated, bright core region exhibiting a yellowish hue, which likely indicates an older stellar population. Moving outwards from the core, the overall light intensity decreases gradually. The outer regions of the galaxy display faint hints of spiral arms. These are not well defined and blend into the diffuse galactic halo. The galaxy appears to be relatively isolated, showing no obvious signs of recent major merging activity, although some subtle disturbances could be present.
