The galaxy presents a generally smooth and rounded morphology, appearing largely featureless upon initial inspection. There is evidence of a central bulge exhibiting a yellowish hue, suggesting the presence of older stellar populations concentrated toward the galaxy's core. Fainter and bluer regions are subtly present throughout the galaxy, indicative of some recent or ongoing star formation activity. While a spiral structure is not immediately obvious, there are hints of disk-like features extending outwards from the central bulge, with very subtle, loosely defined arms that are difficult to discern from the surrounding galactic material. No prominent tidal tails or other clear signs of a recent major merger event are detected, although there is some indication of a minor asymmetry or disturbance in the outer regions, potentially suggesting a minor interaction. Overall, the galaxy is compact in size with a moderate luminosity.
