This galaxy presents as a likely elliptical morphology. The light is centrally concentrated and appears relatively smooth, lacking prominent spiral arms or a well-defined disk. The overall color is yellowish-orange, suggesting a stellar population dominated by older, redder stars with lower rates of current star formation. There is a slight elongation visible, hinting it may be a flattened elliptical galaxy. The galaxy does not appear to be isolated; there are several faint, diffuse features nearby that could be interpreted as tidal tails or debris from a past or ongoing minor merger event. Further spectroscopic data would be required to confirm the galaxy's redshift and the nature of the surrounding features.
