The galaxy presents a largely smooth morphology, with a high degree of central concentration. It appears as a generally round object. There's a notable lack of distinct spiral arm structure or prominent features usually associated with disk galaxies. The galaxy's color profile indicates a dominant yellowish hue, which is consistent with an older stellar population. This color suggests a relatively low rate of ongoing star formation activity. No significant tidal disturbances or merging signatures are readily apparent in the immediate vicinity, implying the galaxy is relatively isolated.
