This galaxy, at a redshift of approximately 0.12, exhibits an irregular morphology. The light profile suggests a dominant, centrally concentrated spheroid. The galaxy displays a generally smooth appearance, yet there is some evidence of disturbed morphology possibly related to a merger or tidal interaction. There are some visible features suggesting recent or ongoing star formation. The color gradients indicate a complex stellar population, with older, redder stars likely contributing to the overall light, and younger, bluer stars concentrated in specific regions. There's a pronounced difference in color and luminosity between the two distinct regions. The inferred size is consistent with a typical galaxy at its redshift. There is a strong indication of an ongoing or past merger event influencing its structure. Overall, the galaxy appears to be in a transitional phase of evolution.
