The galaxy presents as a slightly elongated, luminous object. It exhibits a concentrated central bulge that appears nearly spherical. The bulge region dominates the overall luminosity profile. Extending outwards from this central region is a fainter, more diffuse disk. There appears to be a general smoothness to its overall structure, with limited evidence of strong spiral arms. There might be a subtle flattening along one axis, and a slight asymmetry in the outer regions of the disk, though this could be due to imaging artifacts. The color gradient suggests a transition from relatively older stellar populations in the central bulge to potentially younger populations in the surrounding disk, although the color difference is not strongly pronounced. There are no obvious signs of a major ongoing merger event, although the slight irregularity in shape could be indicative of a minor interaction.
