The galaxy presents an overall smooth morphology, exhibiting a centrally concentrated light profile. The core appears bright and yellowish, indicative of an older stellar population. Moving outwards from the center, the color gradually transitions to a bluish hue in the outer regions, hinting at the presence of younger, hotter stars or perhaps some ongoing star formation. The galaxy's shape is elliptical, with a slight elongation suggesting it is not perfectly spherical. There is no strong evidence of spiral arms or other significant structural features within the galaxy's disk. The overall appearance suggests a relatively evolved system, possibly an elliptical or lenticular galaxy undergoing limited star formation. There are no obvious signs of recent major mergers or tidal disturbances that are influencing the galaxy's overall form.
