The galaxy presents an overall smooth morphology, with a subtle elongation suggesting a possible departure from perfect sphericity. Its color profile indicates a predominantly older stellar population, exhibiting yellowish hues concentrated toward the core. A distinct, compact bluish region is observed offset from the galaxy's center, likely representing a region of more active star formation. There appears to be a degree of tidal interaction or minor disturbance within the galaxy's structure as the shape is slightly off and it is connected to this star forming region.
