The observed galaxy presents a generally smooth morphology. The light distribution is concentrated towards the center, with a gradual fading towards the outer edges. Its shape appears elongated, with a high degree of ellipticity, trending towards a cigar-like appearance rather than a circular profile. There is no obvious indication of a prominent disk structure, although a subtle, flattened component cannot be completely ruled out. The galaxy's color profile suggests a predominantly older stellar population, with a yellow-red hue, particularly concentrated at the core, possibly indicating an abundance of evolved stars. There is no strong evidence of ongoing major merging activity or significant tidal disturbances.
