The galaxy presents as a relatively compact, elliptical object. Its overall color profile exhibits a dominant yellowish-orange hue concentrated towards the core, suggesting an older stellar population. The outer regions show a subtle color gradient, transitioning to slightly redder tones. The shape can be classified as cigar shaped, displaying a significant elongation. There is no discernible spiral arm structure or prominent dust lane features. There is no clear signs of ongoing major mergers or interactions, though potential minor tidal disturbance cannot be completely ruled out from the imaging alone. Based on the general smooth appearance and color distribution, it is plausible to classify this galaxy as an elliptical galaxy, possibly belonging to the earlier morphological types. Further spectroscopic analysis would be required to confirm the age and composition of the stellar population and its precise morphological classification.
