The galaxy presents as an elliptical morphology with a dominant, centrally concentrated bulge. The core region exhibits a bright, yellow-orange hue, indicative of an older stellar population. This contrasts with the outer regions of the galaxy, which display a fainter, more irregular structure with hints of blue, potentially associated with more recent star formation. The shape is generally round, with a low likelihood of cigar shaped. There is some indication of minor disturbances or features, but the overall impression is of a relatively smooth and evolved system. There are no strong indications of a major ongoing merger, but some internal irregularities suggest a possible past interaction. Overall, the galaxy appears to be a reasonably massive system, with ongoing, but relatively low levels of star formation activity.
