This galaxy presents as a centrally concentrated elliptical type object, exhibiting a smooth light profile with no discernible spiral arm structure. The galaxy's core is a bright, yellowish-orange hue, suggesting an older stellar population dominated by red giants. There is a slight elongation observable in the galaxy's morphology, but the overall shape is largely spheroidal. No prominent dust lanes or signs of active star formation regions are clearly visible in this image, reinforcing the likelihood of a passively evolving system. There may be very faint signs of tidal disruption, but no significant merging activity or clear indications of ongoing interactions are apparent.
