The galaxy presents as a relatively small, faint elliptical with an estimated effective radius of about 1.9 arcseconds. Its morphology is predominantly smooth, lacking prominent spiral arms or a distinct disk structure. The galaxy appears moderately flattened, with an approximate b/a ratio of 0.4. Color gradients are evident; the central region exhibits a yellowish hue suggesting an older stellar population, while a slight blue tinge is apparent towards the outer regions. The galaxy displays no signs of major mergers or significant tidal disturbances in the immediate vicinity, although minor irregularities cannot be ruled out with the given image resolution. The Sersic index of 2.9 suggests that the galaxy is of an intermediate luminosity.
