The galaxy presents a mixed morphological profile. A dominant central spheroid appears relatively smooth in texture, with a concentrated core exhibiting a pale yellow hue, likely indicative of an older stellar population. Extending from this core is a fainter, bluish disk-like structure, suggesting the presence of ongoing star formation. This disk component is not as well-defined, appearing somewhat patchy and exhibiting a degree of asymmetry. 

The galaxy displays possible signs of gravitational interaction. There appears to be a secondary concentration of light nearby along with other disturbances, suggesting the possibility of a minor merger or tidal interactions. Some of the observed light may be tidal debris. 

Overall, the galaxy appears to be at an intermediate stage of evolution.