The galaxy appears as a single, concentrated object with a generally elliptical morphology, exhibiting a high degree of central concentration. The light distribution is smooth with no obvious spiral arm structures or distinct features. There is a noticeable colour gradient, transitioning from a bright, yellowish core to a fainter, redder outer region. The general appearance suggests a relatively old stellar population, with a low rate of ongoing star formation. There is no evidence of significant tidal disturbances or interactions with other galaxies in its vicinity. The colour profile indicates a dominant population of evolved stars, consistent with an early-type galaxy.
