The galaxy presents a largely smooth morphology, exhibiting a high degree of central concentration. The overall shape appears nearly circular. There is a slight elongation, but it is minimal. The color profile suggests an older stellar population, with a dominant yellow hue, implying a lack of significant ongoing star formation. No spiral arm structures or prominent dust lanes are discernible. There are no clear signs of tidal disturbances or ongoing mergers, indicating a relatively quiescent state. The light appears to be dominated by the central bulge component, which is bright and well-defined. The outer regions appear fainter and less distinct, gradually fading into the background sky. The galaxy exhibits no irregularities in its light distribution.