The galaxy presents a relatively smooth, elliptical morphology. There is some indication of faint, diffuse features that could be interpreted as a disk-like structure, however it is faint. There is no strong evidence of ongoing merging activity or major disturbances based on visual inspection. The central region displays a somewhat brighter intensity, potentially indicative of an older stellar population. The overall color profile suggests a modest level of star formation, yet with a dominant population of older stars. It is observed to be at a redshift of 0.042401. The estimated stellar mass places it within the realm of a dwarf galaxy.
