The galaxy presents as a slightly elongated, concentrated spheroid of light. Its morphology suggests a relatively smooth structure, with no immediately obvious spiral arms or prominent dust lanes visible in this image. The central region appears brighter and more compact than the surrounding halo, indicating a possible bulge. The overall color profile seems to be trending towards the redder end of the spectrum, potentially indicating an older stellar population and reduced levels of recent star formation. However, there is some evidence of bluer light interspersed within its structure, which could signify ongoing, though perhaps subdued, star-forming activity. There appears to be at least a minor gravitational disturbance within the galaxy, however, no clear signs of merging are present.
