The galaxy appears to be a relatively smooth object with a slight elongation. Its color profile suggests an older stellar population, with a dominant yellowish-orange hue concentrated towards the center. There is little evidence of spiral arm structure or significant dust lanes. The overall morphology leans towards an elliptical or lenticular type, with a high degree of central concentration. Faint, diffuse light extends outwards from the core, gradually fading into the background. There are no clear signs of ongoing major mergers or tidal disturbances, though subtle irregularities in the outer regions could indicate minor interactions. The overall impression is of a fairly massive, evolved galaxy with a low star formation rate.
