The galaxy appears to be an elliptical type. The central bulge is bright and concentrated, exhibiting a yellowish hue, which may indicate an older stellar population. The galaxy's overall shape is elongated, but not highly flattened. Faint, diffuse blue light extends outwards from the core, suggesting the presence of some younger, hotter stars, although star formation appears to be relatively subdued. The galaxy shows no evidence of spiral arms or a distinct disk structure. There are no obvious signs of tidal distortions or mergers. The morphology appears relatively smooth and undisturbed.
