This galaxy presents a relatively smooth morphology, appearing as a somewhat rounded, single structure. The dominant feature is a central bulge, exhibiting a yellowish-orange hue, suggesting an older stellar population. A slight extension or tidal tail emanates from this core, connecting to a smaller, less defined region of bluer light. The blue color suggests recent star formation or a younger stellar population compared to the central bulge. Overall, the galaxy appears to be relatively isolated, although the bluer region might indicate a minor interaction or disturbance that has triggered localized star formation. No strong spiral arm structures or prominent dust lanes are evident. The galaxy is moderately luminous, and appears to be a large galaxy, based on its size.
