The galaxy presents as an elliptical type, exhibiting a smooth, diffuse light distribution, lacking prominent spiral arms or a well-defined disk structure. Its shape appears to be somewhat elongated, leaning toward a cigar-like morphology. The central bulge is quite pronounced, displaying a higher concentration of light compared to the outer regions. The core exhibits a yellow-ish hue, suggestive of an older stellar population. There are subtle hints of bluer light extending from the central region into the surrounding halo, which could indicate the presence of some younger stars or ongoing, but subdued, star formation activity. The galaxy does not show obvious signs of a major ongoing merger, although there could be evidence of minor disturbances in its outer regions or past interactions.
