The galaxy presents as a lenticular or early-type spiral system viewed at an oblique angle. Its overall form is elongated and cigar-shaped with a smooth, relatively featureless appearance, and the galaxy exhibits a noticeable lack of prominent spiral arms or distinct star-forming regions. The central bulge appears to be the most prominent feature, with a higher surface brightness than the surrounding disc. The galaxy displays a smooth light distribution, with the majority of light concentrated in the central bulge region. There are possible subtle indications of a very faint, diffuse disc surrounding the bulge, but these are not clearly defined. There is no obvious evidence of ongoing major mergers, although minor disturbances might exist, the galaxy exhibits a relatively undisturbed morphology. The color index indicates that it likely has a population of older stars and has a redshift of approximately 0.158, implying that it is a relatively distant object.
