The galaxy presents as an elliptical morphology, exhibiting a relatively smooth light distribution. A slight elongation is discernible, suggesting a deviation from perfect circularity. The galaxy's core presents a bright, concentrated luminosity, diminishing gradually towards the outer regions. There is a color gradient, transitioning from a bluer hue near the center towards redder tones in the outskirts, suggestive of varying stellar populations or dust distribution. No distinct spiral arm structures or prominent dust lanes are visible. The overall appearance suggests a galaxy with a population of older stars, particularly in the outer regions. There is a small chance this object is the result of a minor merger. Further spectrographic analysis would aid in determining redshift, stellar composition, and any potential active galactic nucleus activity.
