The galaxy presents a predominantly smooth morphology. It appears elliptical in shape, with a relatively high degree of elongation. There's no discernible spiral arm structure or prominent dust lanes. The light distribution suggests a central concentration, though the resolution limits detailed examination of the core. There is some evidence of minor asymmetry, possibly indicating a past or ongoing interaction, however there are no strong merging features. Based on the color profile, stellar populations are likely to be mixed, containing a large percentage of older stars.
