The galaxy presents an overall elliptical morphology, though with some features suggesting a disk-like component. There is a concentration of light towards the central region, indicating a possible bulge. The color gradients suggest a mixed stellar population; bluer tones are observed within the disk regions which likely denote active star formation, contrasting with the yellower, redder hues concentrated in the central bulge. These redder colors are indicative of an older stellar population. There is evidence of some disturbance within the structure of the galaxy, such as a slightly irregular shape. The observed dust lanes or features may point to recent interaction or merging events. The galaxy appears relatively isolated, though with the slight asymmetry, it could be experiencing some minor tidal disturbance from an unseen neighboring galaxy.
