This galaxy presents a relatively smooth and round morphology. The light distribution appears fairly uniform with a concentrated central region. There is no strong evidence of spiral arm structure or a prominent disk. The galaxy exhibits a color gradient, transitioning from a bluer hue in the outer regions to a more yellow/red hue towards the core. This suggests the central region may be composed of an older stellar population compared to the outer regions. There are no signs of strong tidal disturbances or ongoing major merging events. There is some subtle asymmetry observed, possibly indicating a minor interaction or an internal dynamical process.
