The galaxy presents as a relatively smooth, elliptical-like object, exhibiting a concentrated central bulge that gradually diffuses outwards into a less defined halo. The color profile appears predominantly blue in the central regions, suggesting the presence of younger, hotter stars contributing to the overall luminosity. The blue light transitions subtly towards redder hues in the outer regions, which may indicate an older stellar population. There are no strong indicators of spiral arm structures or prominent dust lanes visible. The overall morphology suggests a galaxy that has undergone, or is undergoing, a quiescent period of star formation, consistent with a spheroidal galaxy classification. The galaxy appears to be relatively isolated, showing no immediate signs of major tidal interactions or ongoing mergers with nearby galaxies, though there is potentially a small disturbance visible. The round shape indicates a lack of significant rotational support, further aligning with an elliptical or S0 galaxy type.
