The galaxy presents an elliptical morphology, appearing somewhat compact with an estimated effective radius of approximately 5.6 arcseconds. Color gradients are noticeable across the galaxy, with a distinctly blue core. This suggests the presence of recent or ongoing star formation in the central region. Moving outward from the core, the colors transition towards redder hues, indicative of an older stellar population in the outer regions. A slight asymmetry may be present, though the low resolution makes it difficult to definitively determine if there is a minor disturbance or a merging event occurring. Overall, the galaxy's light profile appears relatively smooth, though faint, unresolved features cannot be ruled out at this resolution.
