The galaxy presents a generally smooth and rounded morphology. It displays a concentrated central bulge, which exhibits a yellowish-orange hue, suggesting an older stellar population. There is a subtle falloff in surface brightness moving outward from the center, indicating a lack of distinct spiral arm structures. Faint and diffuse bluer regions are observed in the outer edges of the galaxy, which are indicative of possible recent or ongoing star formation. These regions are not well-defined and appear distributed unevenly across the galaxy's periphery. The overall appearance suggests a galaxy with a dominant bulge component and a relatively quiescent star formation rate. There may be signs of some merging activity within the system.
