The galaxy presents as a relatively smooth object, elongated in shape, with a noticeable central bulge. The color gradient transitions from a yellowish-white core to a bluer hue towards the outer regions. This color variation suggests a possible difference in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars populating the disk. There are some subtle hints of spiral arm structures, although they are not well-defined. The overall morphology indicates that this galaxy is likely an intermediate spiral or lenticular type. The edges of the galaxy do not show any obvious signs of ongoing major mergers or significant tidal disruptions. Based on the data, this galaxy appears to be a moderately massive system. Overall, this galaxy appears to be a relatively evolved system.
