The galaxy presents a generally smooth and rounded morphology. The central bulge appears dominant and is characterized by a bright, yellowish hue, suggesting an older stellar population. A faint disk structure is possibly present, exhibiting a bluer tint compared to the bulge, hinting at ongoing star formation. However, this feature is not well-defined. There's no prominent spiral arm structure, which is consistent with the smooth appearance. There is a slight asymmetry in the outer regions, and some faint disturbances may be present, suggesting a possible interaction or past merger event. The galaxy does not appear to be undergoing major merging activity. It presents an estimated mass likely between 10^10 and 10^11 solar masses.
