The galaxy presents as a centrally concentrated object, exhibiting a smooth, largely featureless morphology. The central region appears bright and compact, with a yellowish hue, indicative of an older stellar population. This central concentration fades gradually into a more diffuse, bluish surrounding halo. There's a subtle extension along one axis which could indicate minor tidal disturbance or a slight disk-like structure, although the overall smoothness suggests an elliptical-type galaxy is more probable. There is no indication of spiral arm structure or active star forming regions based on the color or the overall distribution of light within the galaxy. Given the overall appearance and color profile, it is likely that this galaxy has a relatively low star formation rate. The roundness of the galaxy is also suggestive of a more relaxed or evolved system, devoid of major recent merger events.
