The galaxy presents as a relatively compact elliptical type. Its core exhibits a yellowish hue, suggestive of an older stellar population. The light is relatively smooth, with no apparent dust lanes. The galaxy is mostly spheroidal. There are no apparent spiral arms or a distinct disk structure. There is a very faint blue tinge towards the center, indicating a potential small population of younger, hotter stars. There are no apparent tidal tails or signs of recent major merger events. The galaxy shows a moderate luminosity, typical for galaxies at its distance. Overall, the galaxy is a mostly relaxed, spheroid-shaped galaxy with an old stellar population and signs of possible recent star formation.
