The galaxy presents a primarily smooth and elliptical morphology. Its core exhibits a concentrated, yellowish hue, suggesting an older stellar population. Extending outwards from the core, a fainter, more diffuse halo with a slightly bluer tint is observed, possibly indicating the presence of younger stars or ongoing, low-level star formation. The galaxy does not appear to be undergoing any major merging events or showing significant tidal disturbances. It has an overall elongated shape, but not extremely cigar-like.
