The galaxy presents a generally smooth appearance with a slight elongation, exhibiting characteristics between a round and cigar shape. It appears that it is a relatively massive system with moderate ongoing star formation. The overall light distribution is centrally concentrated, hinting at a spheroid-dominated morphology rather than a well-defined disk. The image suggests there might be some minor disturbances in the galaxy's structure, possibly due to a minor interaction or internal processes. The color profile indicates a range of stellar populations, with a dominant population of older, redder stars, along with some regions of bluer, younger stars associated with more recent star formation activity.
