The galaxy presents a generally smooth and rounded morphology. The light is centrally concentrated, exhibiting a bright, yellowish core that fades gradually into a less luminous, slightly redder halo. No distinct spiral arms or bar structures are discernible. The galaxy appears undisturbed, showing no signs of ongoing major merger activity or significant tidal disruptions. The overall color suggests an older stellar population and a relatively low rate of current star formation. Faint, diffuse extensions may be present, contributing to the galaxy's extended profile.
