The galaxy presents an overall smooth morphology, with a prominent central bulge exhibiting a high degree of symmetry. The galaxy's shape appears elongated, deviating from a perfectly circular form. The color profile suggests a dominant population of older stars, particularly concentrated in the central region, indicated by a yellowish hue. Fainter blue regions extend outwards, possibly suggesting some ongoing, albeit low-level, star formation. There is no strong evidence of spiral arm structures, but a subtle disk-like component may be present. No signs of major mergers or strong tidal disturbances are immediately apparent.
