The galaxy presents a generally smooth, elliptical appearance with a high degree of central concentration. The morphology is predominantly spheroidal, exhibiting a relatively round shape. There is no prominent disk structure visible; the light distribution is consistent with an early-type galaxy. The galaxy exhibits a color profile suggesting a population of older stars, with relatively redder hues dominating its overall color. There is no evidence of significant ongoing star formation activity, no obvious spiral arms, or prominent dust lanes. A slight irregularity is visible indicating that the galaxy may be undergoing a very minor merger event. The galaxy appears undisturbed, lacking significant tidal tails or other indicators of a recent major interaction.