The galaxy presents as a moderately luminous, elongated system, approximately 3 kpc in effective radius. Its morphology is primarily smooth, with a possible faint disk structure and evidence of a slight cigar-shaped profile. The central bulge exhibits a bright, concentrated core with a predominantly yellow hue, suggesting an older stellar population. The outer regions display a radial gradient from this yellow-red center towards more blue toned extended features. The galaxy does not appear to be undergoing any major mergers, although it may exhibit minor disturbances within its structure. Star formation rate is inferred to be low given the redder hue. The system's overall appearance is consistent with a late-type spiral galaxy, with some elliptical morphological characteristics.
