The galaxy presents a relatively smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The light distribution is concentrated towards the center, indicating a well-defined nucleus or bulge. The galaxy exhibits a slightly yellowish hue, suggestive of an older stellar population with relatively little ongoing star formation. There is no obvious evidence of any recent merger activity or tidal disturbances. Overall, the galaxy appears to be a quiescent, spheroidal system with a generally uniform structure.
