The galaxy presents a generally smooth morphology, with a dominant central bulge appearing brighter and more concentrated. The overall shape appears somewhat elliptical, though it leans towards being in between round and elongated, lacking a pronounced disk structure. 

Evidence of a minor disturbance can be seen. There appears to be some asymmetry present in its distribution of light, indicating the possibility of a minor interaction or merging event in its recent history. The colors suggest a mix of stellar populations with the central regions exhibiting bluer hues, possibly indicating younger stars or ongoing star formation, while the outer regions have a redder appearance, potentially implying older stellar populations or dust obscuration. The galaxy's estimated size is relatively compact, and the absence of well-defined spiral arms suggests that it is either an early-type spiral galaxy or a lenticular galaxy undergoing morphological transformation. 
