The galaxy presents a somewhat elliptical morphology, appearing largely smooth and relatively featureless. A slight elongation is observed, deviating marginally from a perfectly circular shape. The central region exhibits a bright concentration of light, suggesting a prominent galactic nucleus or bulge. The color profile displays a trend towards redder hues in the core, possibly indicative of an older stellar population. Conversely, the outer regions exhibit a bluer color, which could be due to the presence of younger stars. The overall appearance suggests a galaxy with a moderate redshift, potentially a member of a group. There is some slight asymmetry apparent, perhaps indicative of a minor interaction.
