The galaxy presents as a relatively small, yet distinct, entity. Its morphology appears intermediate between a pure elliptical and a spiral, possibly a lenticular type, but without a prominent bulge. The light distribution is largely smooth, with a hint of a flattened disk. The galaxy exhibits a slightly elongated shape, not perfectly spherical. The color profile suggests a relatively quiescent galaxy with older stellar populations. Faint blueish tinges in the disk may indicate recent star formation, albeit at a low rate. There is no evidence of strong tidal features, major mergers, or significant disturbances in its structure. The galaxy appears to be relatively isolated and undisturbed.
