The galaxy presents as a moderately luminous object with an overall smooth morphology. It exhibits a slightly elliptical shape, appearing more 'in-between' round than distinctly flattened or elongated. There is no clear evidence of spiral arm structure or a prominent disk. The galaxy's color is generally consistent, showing a subtle shift towards redder hues, suggesting a relatively older stellar population. The light distribution is concentrated toward the center, with a gradual decrease in surface brightness moving outwards. There are no obvious signs of major merging activity or tidal disturbances, although minor irregularities in the outer regions cannot be ruled out. The galaxy appears relatively isolated, with no other significant galaxies observed in close proximity.
