The galaxy presents as a relatively compact, elliptical morphology, though there is a slight elongation observable in the major axis. It is a smooth object with no clear spiral arm structures or dust lanes visible. The color appears generally uniform across the galaxy, trending towards the redder end of the spectrum, suggesting an older stellar population with minimal ongoing star formation. There are potential signs of tidal disruption or interactions visible based on it's slight elongation; a plume or faint asymmetrical halo may be present, but it needs further investigation. Given it's apparent lack of distinct features and smooth profile, it would be considered an early-type galaxy. Evidence for any significant merger events requires higher-resolution imaging to confirm.
