The galaxy presents as an elongated structure, appearing to be a disk galaxy seen at a high inclination. The central bulge is not prominently visible. Evident are features suggestive of ongoing interactions or disturbances. The disk appears warped or tidal features are visible. The central core exhibits moderate luminosity. The color profile suggests an active region of star formation throughout the galaxy. The galaxy's overall morphology doesn't strongly align with pure ellipticals but shows more complex structure suggestive of a spiral with irregularities potentially caused by a merger. There seems to be the presence of faint tidal features, which could indicate ongoing or past gravitational interactions. The edges show bluer color.