The galaxy presents a generally smooth morphology, with a spheroidal shape. There is a high concentration of light towards the center, indicating a prominent galactic bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer regions are present in the outer parts of what may be a galactic disk, implying ongoing or recent star formation. No distinct spiral arm structure is apparent. There is very little evidence of any significant tidal disturbances, suggesting this galaxy has not experienced any major recent mergers or interactions. The galaxy appears relatively isolated and undisturbed, with a seemingly settled internal structure.
