The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It exhibits an elliptical-like form, appearing moderately rounded. There is a slight elongation, though not distinctly cigar-shaped. The color gradient suggests an older stellar population, with a yellowish hue, indicative of a population that is no longer actively forming new stars. There is very little indication of internal structures such as spiral arms or a distinct disk component. There appears to be a smaller object adjacent to the primary galaxy, but there is no readily apparent indication of ongoing major merger activity or significant tidal disturbances. There may be a minor disturbance but the smooth structure is more likely.
