The galaxy presents as a smooth, elongated structure, classified as a possible elliptical or lenticular type. It exhibits a bright, concentrated central bulge that appears roughly spherical. Progressing outwards, there is a fading transition to a more diffuse disk-like component. While no prominent spiral arms are visible, slight irregularities in the outer regions indicate subtle structural features or possible tidal disturbances. The color profile demonstrates a redder hue in the central bulge, suggestive of an older stellar population. Conversely, the outer disk appears bluer, potentially indicative of ongoing, although not prominent, star formation activity. The overall morphology indicates a system dominated by ordered motions with a potential mass range indicative of a substantial galaxy. No evidence of recent major mergers is directly apparent; however, there is a slight disturbance in the shape that suggests a minor interaction.
